This galaxy exhibits a distinct spiral structure. The spiral arms appear to be fairly well-defined, with a moderate winding pattern, displaying both medium and loose characteristics. A bar structure traverses the central region. The bulge is neither dominant nor particularly small, suggesting a moderate size. The galaxy's disk is oriented close to face-on. There are indications of ongoing star formation, as suggested by the color profile. The overall morphology appears relatively undisturbed, with no major signs of ongoing mergers, although minor disturbances might be present. Two spiral arms are most common.