The galaxy presents a face-on spiral morphology. Two well-defined spiral arms emanate from a central bulge. The arms appear to be of moderate winding, not tightly coiled, but not exceptionally loose either. The central bulge appears of moderate size. A strong bar structure bisects the central bulge. The arm structures exhibit some bluer regions, indicative of active star formation. There is no immediately apparent indication of a major merger event, but the disk does appear somewhat disturbed, suggestive of a minor interaction or tidal disruption. The overall color gradient suggests a relatively high mass galaxy with ongoing star formation.
