The galaxy presents a distinct spiral morphology, exhibiting a well-defined disk structure. The spiral arms appear tightly wound, emerging from a moderately sized central bulge. Three distinct spiral arms are discernable. The central bulge is a bright, concentrated region, surrounded by a slightly bluer region. No significant bar structure is readily apparent, and the disk appears relatively undisturbed. The arms show a noticeable blue hue. The overall structure suggests a lack of any major ongoing merging events.
