The galaxy presents as a largely featureless elliptical structure. It exhibits a high degree of central concentration and a smooth light distribution, with a consistent falloff in luminosity from the core outward. The galaxy appears nearly circular in projection, indicating a low degree of ellipticity. There is no indication of prominent spiral arms, a bar structure, or dust lanes within the galaxy’s disk. The overall color is consistent with an older stellar population, likely dominated by redder giant stars. There are no discernible features suggesting a recent or ongoing major merger event, however there may be slight disturbances that would be indicative of minor mergers. Overall, this galaxy appears to be a relatively undisturbed, evolved system, dominated by an aging stellar population.