The galaxy presents a generally smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that appears yellowish in color, suggesting an older stellar population. Surrounding the bulge is a less concentrated, more diffuse halo of light. This outer region has a slightly bluer hue than the core, possibly indicating the presence of some younger stars and ongoing, but low-level, star formation. The overall shape is somewhere between round and elongated, but there is no evidence of significant spiral arm structure or a distinct disk. There are no obvious signs of major tidal disturbances or ongoing mergers, although subtle asymmetries may suggest minor past interactions.