The galaxy presents a distinct spiral morphology. The spiral arms are prominent, though somewhat diffuse, appearing lightly flocculent rather than tightly wound. They exhibit a bluish hue, suggesting the presence of young, hot stars and active star formation regions. A central bulge is present, although not strongly pronounced, and appears to be relatively small compared to the overall disk size. A potential bar structure is indicated by a subtle elongation across the central region of the galaxy. There appears to be some indication of a minor interaction or tidal disturbance, with hints of asymmetric outer arm structure. The galaxy is viewed at an oblique angle, allowing a good view of the spiral structure.
