The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a slightly elliptical morphology, appearing more "in-between" round and cigar shaped, with minimal distortion. There is a notable central bulge with a concentrated luminosity gradient. Fainter and bluer star forming regions exist in a loose disk surrounding the central bulge. Some minor tidal disturbance may be present in the outskirts of the disk. Overall, the galaxy appears relatively isolated with no obvious major merging activity.
