The galaxy appears as a relatively compact, elliptical-like structure. Its light profile suggests a smooth distribution of stars, with a high degree of central concentration. There is no distinct nucleus. There is very little evidence of spiral arms or a disk-like structure. The overall color of the galaxy is yellow-orange, indicating an older stellar population that is not actively forming many stars. The light is largely homogeneous and there is no evidence of bright blue star clusters or active star-forming regions, suggesting that the galaxy is not undergoing significant star formation. The overall appearance suggests that this is a relatively massive galaxy. There is no strong evidence of any ongoing major mergers, but some minor disturbances cannot be completely ruled out.
