The galaxy presents as a spiral structure. The spiral arms are prominent, and have a loose winding pattern with relatively wide spacing between them. There are two dominant spiral arms. The central bulge appears relatively small and unobtrusive, it seems to be a classical "bulge", or possibly a pseudo bulge. There is some indication of a weak bar feature in the center. No signs of strong interaction or major mergers, but there is some visible disturbance, possibly a minor interaction with a smaller galaxy. The galaxy's disk is not viewed edge-on, and has multiple features contained within the structure. 