The galaxy presents as a relatively compact, elliptical-like structure. Its light profile is centrally concentrated with a bright, yellowish core that fades gradually outwards. There is little evidence of defined spiral arms or a prominent disk. The galaxy's overall color appears to be on the redder side, suggesting a stellar population that is dominated by older stars and a lower rate of ongoing star formation. There are no obvious signs of major tidal disturbances or ongoing mergers, and the galaxy seems to be relatively undisturbed. The shape is neither perfectly spherical nor highly elongated, appearing more in between round and elliptical.
