The galaxy appears as a relatively compact object with a smooth, elliptical morphology. Its color profile indicates a population of older stars, with a redder hue in the central regions and a slightly bluer color towards the outer edges. There is no discernible spiral structure or distinct dust lanes visible. The overall light distribution is centrally concentrated, with a gradual decrease in intensity outwards. There is no evidence of ongoing major mergers or significant tidal disturbances, though subtle irregularities may be present in the outer halo. The galaxy appears moderately massive.
