The galaxy presents as a relatively smooth, centrally concentrated elliptical morphology. There is a noticeable radial color gradient, shifting from a bluer hue in the core region to a redder color in the outer halo. The galaxy shows no obvious signs of significant disk structure or spiral arms. No major disturbances due to mergers are apparent, although some minor asymmetry could suggest a past interaction. The galaxy is not perfectly round, exhibiting a slight elongation. Overall, the galaxy appears to be a passively evolving system, likely with ongoing, but subdued star formation.
