The galaxy presents as an elongated, edge-on disk galaxy. There is a distinct central bulge with a high concentration of light. The bulge appears to be ovoid in shape. Moving away from the bulge, the disk is visible, with a clear flattening. The light distribution suggests it is a relatively smooth galaxy. The light distribution seems relatively smooth, with light concentrated in the bulge and decreasing towards the outer regions of the disk. The disk appears to be composed of older stellar populations, as indicated by the reddish hue. There is potential evidence of minor disturbance at the bottom of the disk.
