The galaxy presents an overall smooth morphology, with a suggestion of a flattened, disk-like structure. It exhibits a central bulge that appears to be a dominant feature, contributing significantly to the overall luminosity. The shape of the galaxy is somewhere between round and cigar-shaped. There is a possibility of faint spiral arms that are only subtly suggested by slight variations in color and brightness within the galaxy. The color profile shows a central region that is more yellow, hinting at an older stellar population within the bulge. The outer regions appear slightly bluer, which could indicate the presence of younger stars and ongoing star formation, although at a relatively low rate. There is no major interaction evident, although there may be a minor disturbance in the galaxy's structure. Overall the galaxy appears as a relatively undisturbed system with ongoing, but not extremely vigorous, star formation.
