This galaxy presents a prominent disk structure with discernible spiral arms. The spiral arms appear somewhat flocculent and exhibit a medium winding, suggesting an intermediate pitch angle. Some arms show evidence of branching and varying degrees of star formation, indicated by regions of bluer light emission. 

A central bulge is present, though it appears relatively small in comparison to the disk's overall size. A bar structure is evident, extending through the central region of the galaxy. 

There is a clear sense of disturbance in the overall structure. One section of the galaxy shows extended and deformed spiral arms. This disruption may be indicative of a past or ongoing interaction with another galaxy. Overall, the galaxy appears to be actively forming stars, as evidenced by the presence of blue light and somewhat irregular spiral arm features.
