The galaxy presents as a relatively smooth, centrally concentrated object. Its color profile suggests a mature stellar population with a redder hue overall. There is a slight deviation from perfect roundness, presenting as somewhat elliptical in shape, but it is mostly close to round. It appears to be isolated, showing no obvious signs of major tidal disturbances or ongoing mergers, though there might be minor disturbances. Based on its absolute magnitudes, we can deduce it is a massive galaxy undergoing star formation.
