The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing somewhat rounded rather than elongated. The central region displays a bright, concentrated core that gradually fades into the outer regions. There is minimal indication of spiral arm structure or prominent dust lanes. The overall color profile suggests an older stellar population, with a yellowish hue dominating the galaxy's appearance. Subtle irregularities in the outer regions hint at possible minor disturbances, but there is no strong evidence of ongoing major merging activity. The galaxy appears to be relatively isolated, displaying no obvious tidal features or close companion galaxies that would indicate recent or ongoing interactions.
