The galaxy presents a somewhat distorted spiral structure. Distinct spiral arms are visible, appearing moderately tightly wound. The overall morphology suggests a relatively late-type spiral galaxy. The bulge component appears to be minimal. There is a possibility for merging activity, or some form of gravitational disturbance, due to the irregular shape of the arm structures. The galaxy exhibits a bluish hue indicative of ongoing star formation. The galaxy doesn't have a strong central bar structure.
