The galaxy presents as a face-on spiral, exhibiting well-defined spiral arm structures. The arms appear relatively tightly wound, originating from a small, somewhat indistinct central bulge. The arm count appears to be on the higher side, possibly four or more distinct arms can be seen. There are no obvious signs of a strong central bar feature; it appears that no bar exists. The overall disk of the galaxy seems largely undisturbed. There appears to be a slight distortion in the outer edges, suggesting minor gravitational interactions or disturbances may be present, although a major merger is unlikely.
