This galaxy exhibits a prominent spiral structure, possessing well-defined arms extending outward from a central bulge. The arms appear tightly wound, with the majority appearing to fork into multiple spiral arms. Star formation is evident within these arms, as indicated by the presence of bluer regions. The central bulge appears of moderate size in comparison to the overall disk and appears quite bright. There appears to be no strong bar feature present. Overall, there do not appear to be major signs of disturbance due to mergers, but subtle asymmetrical features may indicate a minor gravitational interaction. The galaxy is not viewed edge-on.
