It is known that a Kerr Black Hole (=BH) isn't the same as the Schwarzschild BH viewed from a rotating frame of reference (see here and here). The geometry due to it's "intrinsic rotation" seems to be different from the passive transformation of coordinates viewed with respect to an orbiting test particle around Schwarzschild space-time.
Can we say something similar about a moving BH? There has been perturbative solutions like Aichelburg-Sexl spacetime, Boosted Schwarzschild spacetime , or non-perturbative like in H.Bondi 1962, which involves doing diffeomorphism transformations mimicking Lorentz-boost at infinity. However, they just look like a result of passive transformations w.r.t. observers far away from the source and its not clear what this transformations represent near the massive body.
A related post already exists, but I'm still not sure how to define a "moving BH". It can be wrt observers at infinity (just like in above solutions). However, even a Schwarzschild BH will look like a moving mass wrt orbiting test particle, yet its still Schwarzschild. If the moving particle observes anything similar to the above solutions then qualitatively it should detect gravitational radiations which would constantly decrease the mass of the source. Probably I'm mistaken, but there seems to be some kind of "absoluteness" of a body's state of rest or motion unless the curvature effect is turned off