The galaxy presents as a face-on spiral galaxy, with a prominent central bulge region that appears moderately bright. The spiral arms extending from the bulge are readily discernible, displaying a winding pattern that appears to be relatively medium in tightness, although could also be classified as loose in some areas. The galaxy exhibits two distinct spiral arms. Evidence indicates the presence of a central bar structure spanning across the bulge. Star formation appears present within the spiral arms, and the overall color suggests intermediate population stars. There is no strong indication of interaction or major disturbance. The disk is not viewed edge-on.
