The galaxy presents as a spiral type, with a disk-like structure inclined at a moderate angle relative to the observer. A faint central bulge is present. Two prominent spiral arms are visible extending from the central region. The spiral arms appear loosely wound. No strong bar feature can be discerned. The color suggests active star formation along the spiral arms, giving them a bluish tint. The galaxy is of relatively small size. There is evidence of some gravitational interaction in the form of distortions in the spiral arms. A faint stellar halo surrounds the galaxy.