This galaxy appears to be a spiral galaxy, viewed at an oblique angle but not quite edge-on. There is evidence of a relatively small bulge. The spiral arms are prominent and tightly wound, with high likelihood of two primary arms. These arms appear somewhat flocculent and not particularly well-defined, suggesting ongoing star formation. The disk dominates the overall light profile of the galaxy. There is no readily apparent bar structure. No major mergers are evident, although the overall shape is slightly irregular, implying possible minor interactions or disturbances. The colour suggests that the spiral arms and disk are slightly bluer in colour than the nucleus. 
