This really depends on how close the gamma-ray burst is, and on whether "vaporized" counts as "knocking out of orbit." From the Wikipedia article:
A GRB would be able to vaporize anything in its beams out to around 200 light-years.
If there's a GRB closer than that, not just the mirror but also Earth might be destroyed. So there is plenty of energy to vaporize anything you want!
But suppose you want to push the mirror out of orbit without vaporizing it. Here what matters is how much momentum can be imparted. As the name suggests, the GRB is mostly very high-energy photons - gamma rays. Gamma rays do not penetrate very deeply into solid materials; they will deposit most of their energy in the top few inches of the object. So, if the object is thicker than a few inches, the top layer of the object facing the GRB can rapidly vaporize, producing a reaction force (like a rocket engine) on the rest of the object, which could remain solid and not too damaged. This could be sufficient to push the mirror out of orbit mostly intact, provided the mirror is thicker than a few inches.
The effects would be similar to a nuclear weapon going off in space, which also deposits much of its energy as gamma rays. The GRB lasts a lot longer than the nuclear weapon detonation, but the end result should be similar. See this answer, which includes Python code to calculate the momentum change for a spaceship from its outer hull vaporizing due to incoming radiation.
A burst sufficient to de-orbit a satellite by partially vaporizing it would be very damaging to life on Earth, and would change the orbit of not just the mirror but all smaller objects throughout the solar system.