This galaxy exhibits a complex morphology suggestive of a merger event. The primary body presents a diffuse, somewhat amorphous appearance, with a centrally concentrated region exhibiting a smooth light distribution. There appears to be a secondary, less defined concentration of luminosity nearby, possibly indicating an interaction with another galactic body. The overall shape deviates from a typical elliptical or spiral structure; the galaxy is not perfectly rounded and instead has an irregular form. There is a clear disruption of the overall structure which could be a tidal tail or other signs of interaction, possibly a tidal bridge. The color profile indicates some regions may be actively forming stars, as evidenced by bluer patches, although the overall color is relatively red, implying an older stellar population. The galaxy is relatively faint, indicating either a low luminosity or significant distance.
