The galaxy presents as a face-on spiral system. Spiral arms are observed, displaying a tightly wound morphology, with what appears to be two dominant spiral arms evident. The central bulge exhibits a moderate size relative to the disk, and the galaxy presents no strong evidence of a bar-like structure. No apparent indications of major mergers or significant disturbances in the galactic structure are observed, although there may be some minor disturbances to the disk morphology. The galaxy appears to be dominated by the disk component. The galaxy exhibits a blue color overall, indicative of ongoing star formation.
