The galaxy presents as a spiral type, observed at an oblique angle, but not fully edge-on. A central bulge is visible, exhibiting a yellowish hue, likely indicating an older stellar population. Two distinct spiral arms emanate from the central bulge. The arms are loosely wound and extend outwards, with a bluish tint suggesting ongoing star formation. There are some areas of lower surface brightness within the arms. The morphology suggests no ongoing major merger events. The spiral structure appears relatively undisturbed.
