The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a bright central bulge, with a gradual decline in luminosity towards its outer edges. The color profile suggests a population of older stars, leaning towards redder wavelengths. There is little indication of spiral arm structures or significant dust lanes. The overall shape is generally round, with no obvious signs of major distortions indicative of recent mergers or strong tidal interactions. Star formation appears subdued within the galaxy.
