The galaxy presents a spiral morphology, with a high probability of exhibiting well-defined spiral arms. These arms appear somewhat flocculent, contributing to an overall 'fuzzy' appearance. A central bulge is visible, though it appears relatively small in comparison to the disk. No prominent bar structure is immediately obvious, although there is a possibility of a weak bar present. The disk itself is not edge-on, instead being at an angle that allows the spiral arm structure to be determined. There does not appear to be any evidence of major merging activity or significant tidal disturbance, but minor disturbance can't be ruled out. The galaxy's color suggests ongoing star formation is present within the disk, albeit at a moderate rate. Overall, this appears to be an example of a fairly typical spiral galaxy.