The galaxy appears to be a spiral galaxy, oriented roughly face-on. Its morphology suggests the presence of spiral arms. The arms are not tightly wound, displaying a medium to loose structure. The central bulge is present but appears relatively modest in size compared to the disk. A bar structure may be present within the central region. The overall color is consistent with ongoing star formation, though there appears to be a significant population of older stars, particularly concentrated within the bulge. No signs of major mergers or significant tidal disturbances are immediately apparent in the image, although there may be some minor distortions in the outer disk.
