The object presents as a luminous, elliptical galaxy. The morphology appears largely featureless and smooth, with no distinct spiral arm structures or significant dust lanes readily apparent. The radial light profile suggests a centrally concentrated bulge, with a gradual decrease in luminosity outwards. The overall color index indicates a population of older stars, implying a relatively low current star formation rate. The galaxy exhibits a high degree of circular symmetry in its overall shape. There are no visible signs of ongoing major mergers or significant tidal disturbances.
