The galaxy presents a clear spiral structure, exhibiting tightly wound arms. A dominant bulge is observed, though some of the galaxy may be obscured by interstellar dust. The galaxy appears relatively face-on. A suggestion of a bar-like structure is evident within the central region, bisecting the bulge. The galaxy displays a moderate degree of star formation and appears to be relatively undisturbed, with no obvious signs of a major merger event. There is a possible indication of a minor merging disturbance.
