The galaxy presents as a relatively bright, face-on spiral. Two prominent spiral arms emanate from a central region, displaying a moderate winding. A bar-like structure appears to traverse the central region, exhibiting a notable length compared to the overall size of the galaxy. The central bulge is moderately sized, blending into the inner spiral structure. Patches of varying luminosity are visible along the spiral arms, possibly indicating areas of active star formation. The overall structure appears relatively undisturbed with no obvious signs of major mergers, though some minor asymmetry is noted.
