The galaxy presents a generally smooth and somewhat elliptical morphology, indicating a potential classification as an elliptical galaxy. The light distribution appears concentrated toward the center, suggesting a prominent galactic nucleus or bulge. While generally smooth, the galaxy shows subtle irregularities in its outer regions, hinting at possible past interactions or minor disturbances, although these do not indicate a clear merger event. The galaxy’s color is predominantly yellow-orange, indicating a stellar population dominated by older stars, with relatively low rates of ongoing star formation. The overall structure implies a mature system with a significant mass, situated at a considerable distance.
