This galaxy exhibits a distinct spiral structure, with the spiral arms appearing tightly wound around a central bulge. The central bulge presents a yellow-white hue, suggesting an older stellar population. The spiral arms themselves display a bluer color, indicative of ongoing star formation activity. The galaxy is not viewed edge-on; the disk is significantly inclined relative to our line of sight. There are multiple spiral arms, and although the exact number is difficult to discern, the structure seems complex and somewhat flocculent. The galaxy appears isolated with no signs of major interaction or merging events. There is no evidence of a prominent bar structure crossing the bulge. The overall morphology is indicative of a relatively undisturbed spiral galaxy.
