The galaxy presents as a face-on spiral, exhibiting a well-defined disk structure with a central bulge that appears prominent and smoothly distributed. The spiral arms are clearly visible, tightly wound around the bulge, indicating a grand-design spiral morphology. We can see multiple spiral arms, possibly more than four, branching and winding out from the central region. Patches of blue color are distributed along the arms, suggesting regions of active star formation, while the overall color of the disk is bluer than the bulge. There is no indication of any major mergers or tidal disturbances in this image. Based on the galaxy's morphology, it likely has a significant gas reservoir fueling its star formation activity.
