The galaxy presents a largely smooth morphology, displaying a concentrated central bulge with a radial distribution of light intensity. The light is mostly yellow, though is also appears slightly orange, indicative of an older stellar population. There is no distinct disk structure visible in the image, suggesting it may be an elliptical galaxy. It displays a high degree of circular symmetry, though there may be a slight disturbance from a companion galaxy or an internal phenomenon. The image suggests that the galaxy is not currently undergoing a major merging event. The low level of blue light may be indicative of low star formation activity.
