The galaxy presents a distinct spiral structure. The central bulge appears luminous and somewhat elongated. A bar-like feature is observed bisecting the bulge along its major axis. Spiral arms extend from the ends of the bar, displaying a moderate winding, a relatively tight pitch angle. The galaxy is not viewed perfectly face-on, but at a slight inclination. Patches of star formation or dust lanes are visible along the spiral arms, giving them a slightly clumpy and somewhat mottled appearance. There is no clear evidence of major merger activity, though some minor distortions or asymmetries in the outer regions cannot be ruled out. The galaxy's overall color is somewhat bluish, particularly in the spiral arms, indicating the presence of younger stellar populations.
