The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a bright, concentrated central region, likely indicative of a significant stellar population and potentially a supermassive black hole actively accreting material. The light intensity decreases gradually from the center outwards, with a noticeable absence of prominent spiral arms or distinct features typically associated with disk galaxies. The overall color appears somewhat reddish, suggesting a population of older stars and a relatively low rate of ongoing star formation. The galaxy shows only minor disturbances, possibly due to a small interaction with another galaxy in the distant past, or with no ongoing merging.
