The galaxy presents as a relatively smooth, elliptical structure with a concentrated, luminous core. The morphology suggests an evolved system, potentially an early-type galaxy. The color profile indicates a dominant population of older stars, exhibiting a yellowish-orange hue. There is no discernible spiral arm structure or prominent dust lanes. The galaxy's shape is somewhat elongated but not highly flattened, appearing more "in between" round and cigar shaped. There is no obvious evidence of ongoing major mergers or significant tidal disturbances; the system seems relatively isolated and undisturbed. It exhibits a small degree of star formation.