The galaxy presents as a luminous object with a central concentration, suggesting a substantial spheroidal component. The morphology is largely smooth with a subtle suggestion of extended features. The color profile indicates a mix of stellar populations, with a slightly bluer hue in the outer regions compared to the core. This suggests that the galaxy is not necessarily undergoing a major ongoing interaction or a merger event. There appears to be some asymmetry in the outer regions, which could indicate a past interaction. The smoothness suggests the galaxy is an elliptical galaxy.
