This galaxy presents a distinct spiral morphology. The spiral arms are prominent, and exhibit a tightly wound structure. The disk component dominates the galaxy's overall appearance. There is evidence of a bulge, however it appears to be relatively small compared to the disk. The galaxy displays a high degree of rotational symmetry, with a relatively high axis ratio, suggesting it is close to face-on orientation. The image suggests ongoing star formation as there are hints of patchy, bluer regions within the spiral arms. There is no evidence of any major disturbances or ongoing mergers. There appears to be a weak bar structure in the central region of the galaxy.
