You seem to be thinking of a macroscopic mirror, one whose dimensions are much larger than the wavelength of the emitted black-body radiation. Also, the mirror appears to be smooth enough to have a well-defined focal point. In other words, it is locally flat (almost) everywhere.
In this simple model, the thermal radiation that's locally emitted is going to be uniformly distributed - there's simply no preferred direction. But on a non-local scale, some of the emitted photons may hit the mirror. In turn, some of these may be absorbed, while others are reflected.
Now note that the photons that are absorbed again do not cause local heating. The reason is fairly simple once you realize that light paths are reversible. If a thermal photon emitted at point A hits point B, then thermal photons emitted from B can also travel back to A.
Still, the photons that are emitted at A and reflected at point B will be subtracted from the original uniform distribution, and have a new direction dependent on the angle between the vector AB and the surface normal at point B. For the effects of a single reflection, you'd have to double integrate this over all points A and all points B visible from points A. And of course a photon could be reflected more than once - consider a concave mirror that's shaped like a tube - that's quite similar tp a glass fiber.