The galaxy presents as a face-on spiral, exhibiting a flattened disk morphology. Prominent spiral arms are visible, though their exact number is difficult to discern due to the viewing angle and image resolution. The spiral arms appear moderately tightly wound around the central bulge, with some arms exhibiting clear bifurcation. The central bulge is small compared to the disk size. Evidence of a bar structure is present within the bulge region. The outer disk regions appear somewhat flocculent, with indistinct boundaries. No strong signs of interaction or major mergers are apparent, although some minor distortions may be present. The overall color suggests ongoing star formation activity throughout the disk.
