The galaxy presents as a spiral, though the spiral arms are somewhat flocculent and not particularly tightly wound. There is a distinct, yellowish central bulge, but it does not appear to dominate the overall structure. The galaxy is primarily disk-like, with the spiral arms contributing significantly to its observed morphology. The arms show some clumpy regions of star formation. The galaxy does not appear to be strongly barred, and no major signs of an ongoing merger event are immediately obvious. Some minor disturbances cannot be ruled out.
