The galaxy presents as a somewhat face-on spiral, with a relatively bright, smooth central bulge. The disk appears inclined at a slight angle, showing hints of spiral arm structure. The arms are not well-defined, appearing more flocculent, and demonstrate a color gradient with bluer hues in the outer regions and redder hues concentrated towards the bulge. The overall color suggests a relatively evolved stellar population with ongoing, but not extremely vigorous, star formation. There is no obvious presence of tidal tails or strong morphological disturbances suggesting a major merger event. The disk is relatively smooth and uniform in color. There is some indication of dust lanes close to the central bulge.
