The galaxy presents as a single, relatively smooth object with a concentrated central region. Its overall shape is elliptical, appearing nearly circular from our viewing angle. The galaxy exhibits a radial gradient in luminosity, with the core being significantly brighter than its outer regions. The color profile suggests a population of older stars, with a redder hue dominating the central bulge and a slight blueing towards the outskirts. There is no obvious spiral arm structure or prominent dust lanes visible. No active galactic nuclei are immediately apparent in the core. There are no indications of ongoing mergers or tidal disturbances, though some minor asymmetry in the outer isophotes might suggest a previous interaction. The color suggests it is composed of older stars and is not actively forming many new stars. Based on the concentrated central region, luminosity profile, and color characteristics, it is likely a mature galaxy.
