The galaxy presents as a spiral type, with a noticeable disk component. The spiral arms appear somewhat tightly wound towards the central bulge. Evidence of ongoing star formation is suggested by the bluer colors, with a more prominent, slightly brighter, bulge at the center. The galaxy does not appear to be strongly barred. The disk shows some signs of minor disturbances and has clumpy regions of star formation visible. The galaxy appears moderately inclined from our viewing angle.
