The galaxy presents as a relatively smooth, elliptical-like structure with no clear spiral arm features. It exhibits a concentrated central bulge that appears to be slightly elongated. The color gradient shifts from a yellowish core to a redder outer halo, suggesting a population of older stars dominating the central region, with more recent star formation perhaps occurring in the outer regions, albeit at a low rate. There are no obvious signs of recent or ongoing major mergers, though a slight asymmetry could indicate a minor tidal disturbance or past interaction. Overall, the galaxy appears to be a fairly evolved system.
