The galaxy presents as a spiral type, although the spiral arms are somewhat difficult to discern. The central bulge is prominent and elongated, with a moderate size relative to the rest of the galaxy. Within the spiral arms, regions of active star formation are indicated by their bluer hue. There is a suggestion of a bar-like structure extending from the bulge. The spiral arms appear somewhat flocculent. There is no strong evidence of a major merger event, though some minor disturbances or tidal features may be present.
