The galaxy presents as an elliptical or lenticular type, though with some visible disturbances potentially indicative of interaction or recent merger activity. It appears moderately smooth, with a concentrated central bulge that displays a bright, relatively featureless profile. The galaxy exhibits a noticeable elongation, deviating from a perfect circular shape. The primary color is a pale blue or white, suggesting a population of older stars, although some bluer tints exist, which may signify some ongoing star formation. Distortions are seen in the galactic disk or outer regions that include tidal tails, indicating gravitational disruptions likely resulting from an interaction with another galaxy, or perhaps a past merger event.
