The galaxy presents as a spiral structure, observed at an angle that suggests it is close to face-on. The central bulge exhibits a moderate size and a yellowish hue, indicative of an older stellar population. Spiral arms are clearly visible, displaying a loosely wound morphology. The arms are traced by regions of blue light, hinting at ongoing star formation. There is an apparent absence of a strong bar feature within the central region. The overall structure seems to show signs of interaction or disturbance, however it is relatively minor and is not currently undergoing a major merger.
