The galaxy presents as an elliptical form, with a smooth light distribution that is highly concentrated towards the center. The central region exhibits a yellowish-white hue, indicating the presence of an older stellar population. Moving outwards from the core, the color transitions to a faint bluish tint, which is more pronounced on one side, potentially suggestive of a disk structure or recent, albeit minor, star formation activity. There are irregularities in the outer edges of the galaxy, which appear fuzzy or disturbed. These disturbances may be indicative of minor interactions with another galaxy.
