This galaxy exhibits a clear spiral structure, demonstrating well-defined arms extending from a central bulge. The arms appear tightly wound, suggesting a grand design spiral galaxy. The bulge is relatively small, appearing to be nearly non-existent in comparison to the size of the disk. The disk itself presents a prominent blue hue, indicative of ongoing star formation within the spiral arms. The overall shape of the galaxy is slightly elongated, possibly due to its inherent structure or a viewing angle that is not perfectly face-on. The central region is bright, indicative of an active galactic nucleus or a high concentration of stars. The galaxy doesn't seem to be undergoing any major disturbances or merging events.
