The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a concentrated central bulge that appears yellowish-white, suggestive of an older stellar population. There is a subtle transition outwards from the central region to a more diffuse halo or envelope. The galaxy has an overall round appearance, with no obvious spiral arm structures or strong asymmetries. There is no indication of significant tidal disturbances or ongoing mergers, though a slight irregularity in the outer regions cannot be fully discounted at this resolution. Overall, the galaxy presents a fairly uniform and well-defined structure, consistent with an evolved system.
