The galaxy presents as a concentrated, elliptical morphology, with a smooth light distribution that diminishes gradually from the core. The central region appears bright and yellowish in color, suggestive of an older stellar population, potentially dominated by red giant stars. The galaxy lacks any pronounced spiral arms or distinct features that indicate active star formation on a large scale. There are no apparent signs of a recent major merger, such as tidal tails or significant asymmetries. Faint, diffuse outer regions extend from the central body, possibly composed of older stars or intracluster light. Overall, the galaxy seems to be relatively undisturbed and evolved, characteristic of early-type galaxies found in dense environments.
