The galaxy exhibits a morphology indicative of a system undergoing a major merger. It presents as a single, somewhat amorphous structure with two distinct high luminosity regions. These regions display differing color indices, with one being comparatively redder than the other, suggesting variations in stellar populations or dust extinction. The overall shape deviates significantly from a regular elliptical or spiral form. There is a slight indication of tidal features or extended diffuse emission, however the overall resolution is low. The merging event is likely at an advanced stage, as the two progenitor galaxies are no longer clearly separated, but distinct features remain. The primary light distribution appears relatively smooth, but there is a hint of disrupted structures. Star formation appears to be present.
