The galaxy exhibits a prominent disk structure. The galaxy is face-on, allowing for a relatively clear view of its spiral arms. The spiral arms appear flocculent, with a winding pattern that transitions from medium to loose as they extend outwards from the central bulge. Two spiral arms are particularly visible. The central bulge is moderately sized and appears yellowish. A bar structure appears to bisect the central bulge. There is no obvious ongoing major merger activity, although minor disturbances cannot be ruled out. The morphology indicates active star formation regions.