The galaxy appears to be a relatively smooth, elliptical galaxy. The light distribution suggests a centrally concentrated spheroid with a gradual decrease in luminosity outwards. There is little to no evidence of spiral arms or a distinct disk structure. Its color is suggestive of an older stellar population, with a redder overall hue. The galaxy exhibits a moderate degree of ellipticity, not appearing perfectly spherical, but not significantly elongated. There are no obvious signs of ongoing mergers or tidal disturbances. The lack of clearly resolved features hints at a lack of significant star formation activity, which is consistent with a population primarily composed of older stars. It appears to be a fairly massive system.
