The galaxy presents a generally smooth, elliptical appearance. The central region exhibits a bright, concentrated luminosity, indicative of a significant stellar population and potentially an active galactic nucleus, though the resolution is insufficient to confirm this. The isophotes appear largely regular and concentric. There is a slight elongation observable, suggestive of a mild deviation from perfect sphericity, tending towards a cigar shape. There are no obvious signs of major mergers or significant tidal disturbances. The color gradient suggests a centrally concentrated population of older stars, as evidenced by the yellowish-orange hue. Star formation appears relatively subdued across the galaxy, with a very low star formation rate. Overall, the galaxy appears to be a relatively quiescent, evolved system.
