The galaxy presents as a moderately luminous, fairly smooth object with a slightly elliptical morphology. The light distribution appears concentrated towards the center, suggesting the presence of a central bulge or core. There are no discernible spiral arm structures or prominent dust lanes visible in this image. The overall color of the galaxy appears to be on the redder side, possibly indicating an older stellar population and relatively low ongoing star formation activity. No major mergers or tidal disturbances are apparent, although the possibility of minor interactions or past mergers cannot be completely ruled out based on this image alone.
