The galaxy presents as a single, relatively smooth, elliptical object. It exhibits a concentration of light towards the center, which appears yellowish-white, suggesting a population of older stars. There are no prominent spiral arms or bar structures visible.

The galaxy's overall shape appears somewhat elongated, though not excessively so. There is a subtle color gradient, with a faint bluish-green tinge towards the outer regions, potentially indicating areas of more recent star formation. However, this color is not strongly pronounced, and the overall stellar population appears relatively uniform. There are no clear signs of significant tidal disturbances or ongoing merger activity. The light distribution falls off gradually from the core to the outer edges.
