No, because only electrons, neutrinos and photons will be around
Black holes don't explode; rather, they slowly evaporate - although in the final fractions of a second, they do release substantial amounts of energy. But let's ignore that, and first figure out what the universe will be like by the time this black hole evaporates. A black hole's evaporation timescale is proportional to its mass cubed, $\tau\propto M^3$. For example, a black hole with the mass of our Sun will evaporate in $\sim10^{67}$ years. A supermassive black hole like yours might be like Sagittarius A*, weighing in at about four million solar masses and therefore having an evaporation timescale of $\tau\sim10^{87}$ years.
This, then, is our setting. At this point, we are well into the black hole era of the universe. If protons decay, then by this now all protons and neutrons will be gone; the universe is instead a sea of electrons, neutrinos, their corresponding antiparticles, and photons - and that's it! By the time the black hole evaporates, the universe will be nothing like we know it. There won't even be atoms, let alone galaxies. And those clouds of gas and dust you mentioned? They'll long since have decayed into the same particles. The outside universe will be incapable of forming scientists to observe anything.
The black hole itself won't add much to the universe in the way of matter. The characteristic thermal energy of the black hole, $E_T=k_BT$ (where $T$ is temperature), limits the mass of the particles the black hole can create. For a particle of mass $m$, we would need $E=k_BT\gg mc^2$ to produce such a particle. Even for electrons, this requires rather high temperatures ($>10^9\text{ K}$), which is hotter than most black holes get until the very end of their lives. The black hole will only reach this temperature when it reaches $10^{-17}M_{\odot}$, or about $2\times10^{13}\text{ kg}$; it will evaporate $\sim10^{16}$ years later - a long time on human scales, but only an instance on our timescales. Only in the last 100 million years will it be hot enough to create protons. The vast, vast, vast majority of the particles evaporating black holes produce for most of their lives will be photons and neutrinos.
As a visual aid, here's a plot of $k_BT$ as a function of time until the black hole's evaporation, with lines showing at which points certain particles can first be produced. The neutrino mass is an upper limit, taken from Aker et al. 2019. Keep in mind that this plot is logarithmic! On a linear plot, the three vertical lines would be indistinguishable, smushed together at the extreme far right.
The point is, you can't make much out of an evaporating black hole - let alone astronomers to observe it!