The galaxy exhibits a prominent disk structure. The arms are easily discernible with a strong suggestion of a spiral pattern. The galaxy is not viewed perfectly face-on, but shows some angle of inclination. The spiral arms show a generally organized structure, with some winding. The central bulge is observable but not overly dominant. The disk shows a slight asymmetry; there appears to be a perturbation or some distortion in the morphology suggestive of a minor disturbance. The central bulge color suggest it is older. The arms show regions of more blue which could suggest increased areas of star formation within them. No obvious bar is apparent. The structure looks undisturbed otherwise.