The galaxy presents an elliptical morphology, displaying a smooth, centrally concentrated light distribution. The core region exhibits a yellowish-orange hue, indicative of an older stellar population. Fainter, bluish-white features extend outward from the central bulge, suggesting the presence of some younger stars or regions of ongoing, albeit subdued, star formation. The galaxy displays a slight asymmetry, possibly indicating a minor gravitational interaction or past merger event. There is a hint of a faint tidal tail or extended structure on one side of the galaxy, further supporting the possibility of a past interaction. The overall structure appears relatively undisturbed, suggesting that any interaction was not recent or particularly violent.
