The galaxy presents a generally elliptical morphology with a smooth, diffuse appearance, suggesting a lack of significant spiral arm structure or prominent dust lanes. The color profile indicates a population of older stars dominating the light output, with a redder core transitioning to slightly bluer hues in the outer regions. The galaxy appears relatively undisturbed, showing no obvious signs of recent major mergers or tidal interactions. The central bulge is well-defined but not exceptionally bright, and the overall light distribution is moderately concentrated. The galaxy's shape appears somewhat elongated, with a ratio of major to minor axis greater than 2:1. There is a slight asymmetry in the light distribution, with one side appearing slightly brighter than the other.
