This galaxy exhibits a distinct spiral structure, although the arms appear somewhat flocculent and not sharply defined. Two spiral arms seem to dominate the structure. The winding of these arms appears to be of medium tightness. The central bulge is prominent and of moderate size relative to the disk, displaying a yellowish hue indicative of an older stellar population. The disk itself exhibits a bluer color, suggesting ongoing star formation. There is no apparent bar structure. The overall appearance of the galaxy does not show any major signs of recent or ongoing mergers, but there seems to be a slight asymmetry in the shape of the disk.
