The galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears predominantly elliptical or lenticular, displaying minimal discernible disk-like features. The light distribution is characterized by a bright central bulge which gradually decreases radially. The color gradient suggests a population of older stars dominating the central region, indicated by the yellowish hue. The outer regions exhibit a bluer tint which could be attributed to some ongoing star formation within these areas, although at a relatively low rate. There is a subtle suggestion of minor disturbances in the morphology, hinting at potential past or ongoing minor interaction events. No strong tidal features or signs of a major merger are immediately apparent. The overall structure suggests that the galaxy is fairly mature, with a relatively high stellar mass.
