The galaxy presents as a face-on spiral galaxy with a prominent disk. The spiral arms are well-defined, displaying a predominantly two-arm structure. The winding of the spiral arms appears to be of an intermediate type. A bar structure is subtly visible within the central region, though it does not appear particularly strong. The central bulge seems moderate in size, contributing significantly to the overall brightness of the galaxy's core. Patches of blue star formation are observed within the spiral arms, indicating ongoing stellar genesis. The galaxy shows no obvious signs of major mergers or significant disturbances, appearing relatively isolated and undisturbed. 
