The galaxy presents as a spiral type, displaying a notable disk component. Two well-defined spiral arms are visually apparent, exhibiting a moderately wound morphology. A central bulge is present, appearing to be of moderate size relative to the galactic disk. A bar-like structure seems present traversing the central bulge, but the strength of the bar is difficult to ascertain based on the image alone. There is no clear evidence of major disturbances in the galaxy's structure, but a minor disturbance is possible. The galaxy is not viewed edge-on, but at a slight angle that allows the disk and spiral structure to be seen. The general color gradients suggest ongoing star formation within the spiral arms.
