The galaxy presents as an elliptical-type structure with an overall smooth appearance. The core region exhibits a bright, concentrated luminosity, suggesting a high stellar density. The light profile appears to decrease gradually outwards from the center, lacking distinct spiral arms or a well-defined disk. The galaxy displays a reddish hue, indicating a population of older stars and/or significant dust obscuration. There are possible signs of tidal disturbances, although the galaxy is predominantly exhibiting a centrally concentrated mass. Close inspection reveals very faint extensions that can be interpreted as low surface brightness regions. The galaxy exhibits moderate ellipticity, and possible minor signs of a recent or ongoing minor merger. The dominant appearance suggests a smooth, undisturbed morphology.
