Your black hole has a horizon radius round about $1\times10^{-15} $ meters. That's round about 100,000th of the width of a Hydrogen atom. The mass you suggest, $3.98 \times 10^{11}$ kg is, on a planetary scale, kind of small. Mount Everest comes in at about $8 \times 10^{14}$ kg, two thousand times as big.
Example calculation of bending of light by the Sun.
Bending is proportional to the mass and inversely proportional to the minimum radius the light passes by. The Sun with $2\times10^{30}$ kg mass, produces at a min approach distance of 700,000 km, $8.5\times 10^{-4}$ degrees of deflection. To get 1 degree of deflection with your mass, the light would have to pass within $1.18\times 10^{-13}$ meters of your black hole. That is round-about one thousandth the width of a Hydrogen atom.
Your blackhole will be more-or-less invisible to your laser beams. The tidal effects could be interesting, but I didn't work them out. For purposes of laser shots it will be utterly useless. Indeed, unless you get close enough for the tides to be meaningful (probably within a couple meters) you'd be hard pressed to find it.
Except! Except for the Hawking radiation. A black hole with this mass has a useful life span in the billions of years. But it has a nominal luminosity of 2 billion Watts. So the BH itself will be putting out this incredible amount of radiation, probably more than any laser beams you could hope to mount on a spaceship. The upper end of particle energy is round about 100 MeV electrons, which is very nasty indeed. It's not in a beam, but still, you don't want to get too close.
Black Hole Hawking Radiation Calculator