The galaxy presents as a spiral galaxy viewed at an oblique angle relative to its disk. There is a noticeable central bulge region, though it does not appear to be the dominant feature. The spiral arms are prominent, with what appear to be two primary arms. The arms appear loosely wound. There are indications of star formation within the spiral arms, particularly at the leading edges, suggesting regions of higher density and compression. There appears to be a weak bar structure crossing the central bulge. There is a notable amount of disk disturbance; the galaxy appears to be potentially interacting or merging. The light distribution suggests this is a blue galaxy, suggesting active recent star formation.
