The galaxy presents as a generally smooth, disk-like structure. It exhibits a prominent central bulge, appearing bright and concentrated. The outer disk shows a bluer hue compared to the bulge, indicating the likely presence of younger stellar populations. There is a slight suggestion of spiral arm structure or perhaps patchy star formation within the disk, although they are not well-defined. The overall shape appears mildly elongated, deviating slightly from a perfect circle. There's no obvious sign of a major merger event, though there are some minor disturbances present. The object is generally considered to be smooth with some features, though not an artifact. It is considered to be relatively unmergered, though there is some signs of minor disturbance. The galaxy is likely moderately massive and has a low star formation rate.