The galaxy exhibits a prominent spiral structure, with well-defined arms emanating from a central bulge. These spiral arms appear somewhat patchy and flocculent. The central bulge is distinct, appearing as a bright, concentrated region. The galaxy's disk is observed face-on, allowing for a clear view of its spiral morphology. There is no obvious indication of a strong bar feature. The overall color suggests ongoing star formation, particularly within the spiral arms. Indications of some minor disturbances are present, possibly due to interactions or mergers. 
