The galaxy presents as a spiral type, exhibiting distinct spiral arm structures. The arms appear relatively well-defined, emanating from a central bulge region. The winding of these arms tends toward a medium tightness. The bulge is of moderate size relative to the overall disk of the galaxy. There is no discernible bar structure visible in the central region. The overall disk appears relatively undisturbed, showing no significant signs of a major merger event. Star formation is evident within the spiral arms, contributing to their blue hue. A relatively smooth, yellow core can be seen at the center of the galaxy.
