The galaxy presents as a spiral type with a prominent disk structure. The spiral arms are well-defined and appear tightly wound around the central bulge. A bar-like structure is also visible.

The central bulge exhibits a moderate size and is characterized by a smoother, more concentrated light distribution compared to the disk. The disk shows distinct color variations, potentially indicative of ongoing star formation activity, particularly in the spiral arms. Dust lanes may be present within the spiral arms.

There does not appear to be any significant interaction with another galaxy. The general morphology suggests a system that is relatively undisturbed.
