The galaxy presents as a relatively smooth and rounded structure. It exhibits a noticeable central bulge with a yellowish-white hue, suggesting a population of older stars. The outer regions appear less concentrated with a bluer tint, potentially indicating the presence of younger stars or ongoing star formation. There are no obvious spiral arms or a pronounced disk. Faint irregular features or tidal tails are not discernible, suggesting minimal interaction with other galaxies. Overall, the galaxy appears as an elliptical galaxy with a relatively high mass and moderate luminosity. Star formation rates are low, indicating that the galaxy is not particularly active in forming new stars.
