The galaxy exhibits a clear spiral morphology. The spiral arms appear tightly wound around a prominent central bulge. The bulge component seems relatively small in comparison to the overall disk size, but is bright. The arms themselves appear grand design, with an organized and symmetric structure. There may be at least three spiral arms identifiable. Star formation regions are present within the arms, visualized as regions of bluer color, contrasted against a more yellow-red background indicative of older stellar populations. There is no obvious sign of a bar structure in the inner region.
