This galaxy presents a clear spiral structure. Two prominent spiral arms are visible, originating from a central bulge, and winding outwards with a moderate pitch angle. The bulge appears relatively small in proportion to the overall disk size. The arms display clumpy structures, suggesting active regions of star formation.  The bluer hues observed in the arms are indicative of a younger stellar population. The disk is viewed at a slight angle from face-on, providing a clear view of its spiral morphology. There is no apparent major disturbance or ongoing merger evident in the image, though some minor asymmetry is visible.
