The galaxy exhibits a prominent spiral structure. Tightly wound spiral arms emanate from a moderately sized central bulge. The arms appear somewhat patchy, indicating regions of active star formation. The galaxy is not perfectly face-on but shows some inclination. There is a hint of a bar-like structure extending from the central bulge. There is no obvious major ongoing merger, though minor disturbances may be present. The disk component dominates, appearing relatively smooth, but with areas of higher and lower surface brightness.