The galaxy appears to be a spiral galaxy, although the arms are somewhat indistinct. It presents a disk-like structure with a noticeable central bulge. The galaxy's orientation is somewhat face-on, allowing us to observe its overall shape. Patches of blue are visible within the galaxy, suggesting regions of active star formation. The presence of a bulge indicates a concentration of older stars toward the galactic center. Overall, the galaxy appears to be of moderate size with evidence of both younger and older stellar populations.
