The galaxy appears as a somewhat diffuse object. It presents a disk-like morphology with a central bulge. Evidence suggests this is an actively star-forming system. The galaxy exhibits what appears to be a significant disturbance, likely from a merger event. There is an obvious distortion in its structure, with hints of tidal tails and possibly more than one distinct center of luminosity. The presence of an active galactic nucleus cannot be ruled out. The system is not particularly blue and is actively forming stars.
