The galaxy presents as a smooth, elliptical-like structure. Its light profile suggests a centrally concentrated bulge, with a gradual decrease in intensity towards the outer regions. There is little evidence of spiral arms or significant dust lanes, implying a more evolved system. The color of the galaxy appears to be generally yellowish, which indicates a population dominated by older stars and a relatively low rate of ongoing star formation. No clear signs of active galactic nuclei or starburst activity are visible, based on this image. The overall morphology suggests a relatively undisturbed galaxy that is unlikely to be undergoing a major merger or significant interaction with other galaxies.
