The galaxy presents a disk-like structure with a prominent central bulge. The spiral arms appear tightly wound and somewhat flocculent in nature, with no apparent grand design. Light from the galaxy is dominated by what appears to be slightly longer wavelengths. It's apparent that the blue emission is less dominant than the red emission. There is some indication of a bar feature within the central region, although it is not distinctly visible due to the moderate bulge size. The galaxy shows no strong signs of tidal disruption or major mergers, but some minor disturbance or interaction is not ruled out. The disk appears to be viewed at an angle, but not fully edge-on.
