The galaxy presents as a relatively faint, elongated structure in the image. It appears to be an edge-on or nearly edge-on disk galaxy. A prominent central bulge is visible, appearing somewhat rounded. The disk component shows a faint orange hue, possibly indicating an older stellar population. Some degree of internal structure within the disk may be present, but its detail is limited by the image resolution. There is no obvious evidence of a recent major merger or significant tidal disruption.