The galaxy presents as an edge-on disk galaxy. A prominent dust lane bisects the disk horizontally, obscuring the central bulge region. The bulge appears somewhat rounded. The disk exhibits a slight reddish hue, potentially indicative of older stellar populations or dust reddening, with a detectable level of ongoing star formation. There are no obvious signs of a major merger or tidal disturbance, although a minor disturbance cannot be ruled out.
