The galaxy presents as a primarily smooth, centrally concentrated object. Its overall shape is more elongated than circular, appearing somewhat elliptical. There is a bright, relatively compact core that dominates the luminosity profile. The color gradient suggests a population of older stars, given the tendency toward redder colors. The galaxy does not exhibit any obvious spiral arm structure or prominent dust lanes. There is a faint, diffuse halo surrounding the central region, which smoothly blends into the background sky. The general appearance suggests a relatively quiescent galaxy with low ongoing star formation. It appears to be largely undisturbed, showing no strong indications of a recent merger or interaction.
