The galaxy presents as a relatively face-on spiral, exhibiting a dominant disk structure. Spiral arms are clearly visible, and tightly wound around the central bulge. While the bulge itself is discernable, it appears small in comparison to the overall disk size, suggesting a later-type spiral morphology. Some indications of active star formation regions are suggested by the presence of some faint blueish spots in the spiral arms. The overall color of the galaxy is indicative of a more evolved stellar population. The image doesn't show evidence of tidal tails or strong morphological disturbances, suggesting the system is relatively isolated and unperturbed. However, some minor disturbance cannot be ruled out completely, given the slightly irregular appearance of the spiral arms in some parts of the galaxy. No bar structure is obviously apparent. The central bulge appears smooth and spheroidal.
