The galaxy presents as a relatively smooth, centralized structure, exhibiting a largely elliptical morphology. The light distribution is concentrated toward the center, with a gradual fall-off in surface brightness moving outwards, indicating minimal or no presence of prominent spiral arms. There is an absence of any distinct dust lanes or regions of active star formation. The overall color appears to be slightly red, suggestive of an older stellar population. The galaxy appears to be isolated, without obvious signs of tidal interactions or ongoing mergers with nearby galaxies, although there are some small artifacts nearby. Overall, the galaxy appears consistent with a mature elliptical galaxy.
