The galaxy presents as a face-on spiral, exhibiting a prominent and bright central bulge. The spiral arms are well-defined and tightly wound, displaying a generally symmetrical structure. Two main arms are discernible, with hints of further arm segmentation. The arms exhibit a bluer hue, indicating regions of active star formation. The bulge appears yellowish-white, suggesting an older stellar population. The overall structure suggests a relatively undisturbed morphology, with some indication of minor irregularities within the arm structure. The disk is not edge-on, and there is no obvious bar structure extending from the bulge. The spiral arms appear to merge smoothly into the central bulge, and a notable fraction appear tightly wound. There are no obvious signs of a major merger or tidal disturbances.
