This galaxy exhibits a distinct spiral morphology. Two dominant spiral arms are readily apparent. The winding of these arms appears moderately open. The central bulge appears relatively bright with a yellow hue. The disk appears bluer, suggesting active star formation. Overall, the galaxy appears relatively undisturbed, showing no prominent signs of a major merger, though a minor interaction cannot be ruled out. The orientation of the disk is not perfectly face-on, but is close, providing a clear view of the spiral structure. There is evidence of a weak bar structure in the galaxy's center.
