This galaxy exhibits a pronounced disk structure with tightly wound spiral arms. There is a notable central bulge, appearing relatively smooth and bright, possibly indicating a high stellar density. The galaxy is observed at an angle, showing a slight ellipticity to its overall shape. The disk appears relatively smooth, possibly dusty, and exhibits a bluer color than the central bulge, indicative of ongoing or recent star formation. The galaxy does not appear to be undergoing any major merging events or significant tidal distortions, suggesting it is relatively undisturbed.
