The galaxy exhibits a spiral morphology, with a moderate bulge size relative to the disk. The spiral arms are tightly wound around the central bulge. Evidence suggests that the galaxy is relatively undisturbed, showing no signs of major merging activity. The disk is not edge-on; we are seeing it at an angle. The galaxy exhibits a clear color gradient, with the central bulge appearing more yellow, while the outer disk and spiral arms appear bluer. The overall shape is somewhat elliptical. There may be a very weak bar structure present, though this is hard to determine.
