The galaxy presents as a spiral morphology, exhibiting prominent, well-defined arms. The arms are relatively tightly wound and appear to originate from a central bulge region. The bulge displays a moderate size relative to the overall galaxy. A bar structure is visible, though its strength appears moderate rather than dominant. Two spiral arms are clearly present.

Evidence suggests potential ongoing or recent interactions or merger events. There are visible distortions within the spiral structure, with notable asymmetries in the arm structure.

The disk is viewed at an angle between edge-on and face-on.
