The galaxy presents a spiral structure, exhibiting well-defined arms that extend from a central region. The arms appear somewhat fragmented and less tightly wound, suggesting a flocculent or grand design spiral morphology. The presence of a bar-like structure is implied by a slight elongation in the central region.

The bulge component appears relatively small compared to the overall disk, though its morphology isn't perfectly clear given the viewing angle. Star formation appears moderately active within the spiral arms, evident through regions of bluer luminosity. No signs of strong interactions are apparent, although there seems to be some distortion in the overall shape. The galaxy's light profile indicates a relatively smooth transition from the central bulge to the outer disk.
