This galaxy presents a distinct disk-like morphology, observed at an oblique angle. The central bulge region appears relatively small but bright, exhibiting a yellowish hue, indicative of an older stellar population. Extending outwards from the bulge are prominent spiral arms.

These spiral arms exhibit a clumpy structure, suggesting regions of active star formation. The overall color gradient shifts from yellow-white in the central bulge to a bluer tint in the outer spiral arms, consistent with the presence of younger, hotter stars in the arms. Dust lanes are faintly discernible within the spiral arms, obscuring some of the starlight. The overall shape and arm structure indicate a relatively high degree of order within the galaxy.
