The galaxy presents as a spiral type, characterized by the presence of distinct spiral arms. While a prominent central bulge region is observed, it doesn't dominate the overall morphology. The spiral arms exhibit a moderate winding, neither tightly wound nor loosely defined. Two primary arms are discernible, with some indication of branching and additional arm segments. Patches of intense blue light are distributed within the arms, potentially indicating regions of heightened star formation activity.

There appears to be an asymmetrical structure in the galaxy. On one side, the spiral arm is much more pronounced and has a more prominent blue color.
