The galaxy presents a distinct spiral morphology, exhibiting well-defined arms emanating from a central region. The spiral arms are moderately wound, displaying a blend of both tight and loose structures. There is evidence of at least three and possibly four distinct spiral arms. The central region has a prominent bulge. A bar structure is not immediately apparent. The disk appears face-on, as no significant inclination is observed. Signs of interaction are visible in the spiral arms. The system displays a notable blue tint, suggestive of recent or ongoing star formation activity. Overall, the galaxy exhibits a complex and dynamic structure indicative of an evolving spiral system.