The galaxy presents as a spiral galaxy. It exhibits a moderate-sized bulge, appearing somewhat elliptical and centrally concentrated. The spiral arms are prominent. The winding of the arms appears to be relatively loose, and there are two dominant spiral arms that wrap around the galactic center. There is evidence for a strong bar structure that bisects the central bulge region. There does not appear to be evidence of any major mergers occurring. The galaxy appears relatively undisturbed, although there is a hint of asymmetry.
