The galaxy presents as a somewhat diffuse spiral galaxy. It has a moderate-sized bulge that does not dominate the overall structure. The disk exhibits clear spiral arm structure that is neither tightly wound nor significantly disrupted. There is no bar structure visible. The galaxy is not undergoing any major merging activity and appears relatively undisturbed. The presence of a bulge and spiral arms suggest that star formation is ongoing within the galaxy, though possibly at a low rate. There is not significant colour variation throughout the galaxy. 