The galaxy presents a distinct spiral morphology. The spiral arms are tightly wound, extending outwards from a central, bright, but relatively small bulge. The disk appears to be viewed nearly face-on. The galaxy is not perfectly symmetrical. The light distribution in the arms is notably clumpy. The spiral arms show some evidence of active star formation, indicated by their subtle blue tint, but the galaxy, overall, has a smooth appearance. The galaxy shows no obvious signs of recent major merger activity or strong tidal disruption, although there are minor disturbances. A faint bar might be present, bisecting the central bulge but this is ambiguous. The galaxy is likely not an edge-on disk galaxy. The dominant component is the disk, with a small contribution from a bulge. The number of clearly identifiable spiral arms is difficult to discern, but the features are overall quite tight and distinct.
