The galaxy presents as a moderately luminous object, exhibiting an apparent angular size suggesting a physically large scale. It exhibits a morphology suggestive of a major merger event or interaction. A significant fraction of the light appears concentrated into two distinct, bright nuclei or clumps, indicating either two distinct galaxies in the process of merging, or significant asymmetrical star formation within a single galaxy. There appears to be a diffuse, extended envelope of fainter material surrounding the primary components, hinting at tidal debris from the ongoing interaction. The galaxy's color profile indicates a significant population of evolved stars contributing to the overall luminosity; colors are largely redder, but are noticeably bluer in some regions. The galaxy's shape is significantly distorted and not readily classified as a typical elliptical or spiral.
