The galaxy presents a largely smooth, elliptical morphology. The core region exhibits a bright, concentrated luminosity, indicative of a high stellar density. The overall color is yellowish, with hints of red, suggestive of a population of older stars. The galaxy has a somewhat rounded shape, without a distinct disk structure. There are two relatively symmetrical disturbances visible to the right and left of the galaxy, they appear to be much smaller and less luminous than the main galaxy. The absence of obvious spiral arms or significant dust lanes further reinforces its classification as an elliptical galaxy. No significant tidal features or indications of a major ongoing merger are apparent, though the possibility of a minor past interaction cannot be ruled out based on the disturbances.
