The galaxy presents as a relatively compact, elliptical morphology with a smooth, centrally concentrated light distribution. There is no discernible spiral arm structure or dust lane. The galaxy exhibits a color gradient, appearing more yellowish-orange towards the core and subtly bluer towards the outer regions. The overall color suggests a stellar population dominated by older stars, though the bluer periphery indicates the presence of at least some younger, hotter stars and thus ongoing star formation. There is no strong evidence of tidal disturbances, major mergers, or significant morphological irregularities. The isophotes appear generally regular and elliptical, but are still not perfectly circular. The galaxy appears relatively isolated within the field of view, with no nearby companions that are obviously tidally interacting with it.
