The galaxy exhibits a prominent disk structure with visible spiral arms. The arms appear somewhat patchy and are not tightly wound, displaying a more open morphology. There is evidence of active star formation within the spiral arms, indicated by the presence of numerous bright, blue knots likely representing young star clusters or HII regions. The central bulge is relatively small and does not dominate the overall structure of the galaxy, and it is not particularly bright. Overall, the galaxy displays characteristics of a spiral galaxy with ongoing star formation and a relatively low central mass concentration.
