The galaxy presents a complex morphology, appearing as a spiral type when viewed face-on. Prominent spiral arms are visible, although their definition is somewhat diffused. There appears to be a central bulge which is moderate in size. A weak bar structure may be present traversing the galactic center. Some disturbances within the disk and spiral arms suggest possible minor interactions or ongoing mergers. Color gradients across the galaxy indicate varying stellar populations and dust content. The system displays a diverse range of colors, suggestive of ongoing star formation, which is potentially driving the disturbances seen in the disk.
