The galaxy presents as a somewhat elongated, elliptical form. Its core region is intensely luminous, exhibiting a yellowish-white hue, suggesting a population of older stars dominating the central bulge. The light diminishes gradually outward from the core, forming a diffuse halo. There is a hint of a disk-like structure, viewed at an angle. Faint reddish regions are observed towards the edge of the galaxy, potentially indicating areas of ongoing or recent star formation, though this activity appears minimal. The overall structure appears relatively smooth with some minor disturbances that could indicate a past interaction or tidal effects. The galaxy does not exhibit any strong spiral arm structures.
