The galaxy presents as a dominant, centrally located elliptical structure. It exhibits a smooth light distribution with minimal visible substructure. Its morphology appears largely undisturbed, showing no signs of major mergers or significant tidal interactions. The galaxy's color profile indicates a population of older stars, with a redder hue dominating. The roundness of its overall shape is apparent and there is no indication of a disk. The lack of prominent blue regions suggests a relatively low current star formation rate.
