The galaxy exhibits a prominent disk structure, oriented face-on relative to our line of sight. The spiral arms are well-defined and appear grand-design in nature. The galaxy has a central bulge, which appears moderate in size and exhibits a smooth texture, which transitions into the disk gradually. The galaxy shows moderate star formation activity, indicated by the presence of blue regions associated with the spiral arms, signifying the existence of massive, young stars. There is evidence of a bar structure in the central region of the galaxy, appearing subtle. Overall, the galaxy appears to be relatively undisturbed with no major signs of recent or ongoing mergers.