The galaxy presents as a moderately bright, elliptical-shaped object with a concentrated central bulge. The light distribution appears relatively smooth, with a gradual decrease in intensity from the core outwards. There is a subtle color gradient, the central region appears more yellow/golden, potentially indicating an older stellar population. The outer regions are slightly bluer, suggesting some ongoing, but low-level star formation. No distinct spiral arms or prominent dust lanes are visible. There is no strong evidence of a major ongoing merger event, however, there is some minor asymmetry in the outer profile, potentially indicative of a past interaction or minor disturbance.
