The galaxy presents as a yellowish, moderately luminous, and centrally concentrated object. There is a suggestion of a disk-like structure, though this is not sharply defined. It appears mostly smooth with slight hints of irregular features and disturbances. There is no definitive spiral arm structure visible. The overall color suggests an older stellar population dominating the light output, possibly with ongoing merging events in its recent history. The galaxy has a generally elliptical shape, though deviations from perfect ellipticity are apparent, possibly indicating tidal interactions or recent merger activity. The blurring around the core may indicate active star formation, though its low star forming rate indicates it is in the process of dying.
