The galaxy presents as a spiral with a prominent central bulge. The bulge exhibits a yellow-white hue. The spiral arms appear fairly well-defined and extend outwards from the central bulge, displaying a bluish tint indicating younger stellar populations. The arms show a relatively loose winding pattern, with two arms clearly visible. There is evidence of star formation within these arms. The galaxy displays a slight inclination relative to the observer's line of sight. There is a weak indication of a bar structure. The morphology suggests a galaxy that is undergoing active star formation.
