The galaxy exhibits a spiral morphology. Two prominent spiral arms are visible, displaying a moderate winding. A faint, relatively small bulge appears at the galactic center. The disk appears to be oriented close to face-on. There are disturbances visible in the disk. The central region displays a smoother, more concentrated light distribution suggesting an older stellar population, while the outer regions show bluer colors, indicative of ongoing star formation. The galaxy's overall shape is slightly elliptical.
