The galaxy appears to be a spiral galaxy, oriented at an oblique angle relative to the line of sight. It exhibits a prominent disk structure, with tightly wound spiral arms emanating from a central bulge. The bulge appears relatively small, with a moderate concentration of light. The spiral arms are well-defined and show evidence of active star formation, as indicated by the presence of blue regions interspersed throughout the arms. These blue regions are indicative of the presence of hot, young stars. The overall color of the galaxy is slightly blue, suggesting ongoing star formation activity. There is no obvious presence of a strong bar feature across the bulge. No signs of any ongoing major merger can be seen.
