This galaxy appears to be a spiral galaxy viewed at a slight angle, not quite face-on. It exhibits distinct, though somewhat loosely defined, spiral arms. The central bulge is not particularly prominent, appearing relatively small and indistinct compared to the overall disk size. The overall color of the galaxy is bluish, suggesting a significant population of young, hot stars, and therefore ongoing star formation. There appears to be some degree of disturbance in the galactic morphology, possibly indicative of tidal interactions or a past merger event. There is no clear evidence of a strong central bar structure. 
