The galaxy presents a distinct spiral structure, exhibiting well-defined arms emanating from a central bulge. The spiral arms appear flocculent and demonstrate a moderate winding, suggesting an intermediate stage in their evolution. Two prominent spiral arms can be easily distinguished, with hints of additional fragmented arms.

A bar-like structure is present across the galaxy's center, with a significant portion of the galaxy appearing to be influenced by the bar. The central bulge is relatively prominent, contributing significantly to the overall light output of the galaxy. The galaxy displays a varied morphology, with some regions suggesting possible disturbances, although the main structure remains relatively intact.
