The observed galaxy presents as a lenticular or possibly an edge-on spiral galaxy. The overall morphology appears relatively smooth, with a central bulge that is bright and appears slightly blue-white. There is a visible disk component with some indications of dust lanes. The disk appears elongated, giving the galaxy a cigar-like shape. Faint red or orange hues appear toward the far edges of the disk, indicating regions of likely older stellar populations or dust obscuration. There is a possible minor disturbance in the disk. No clear spiral arm structure is evident, which may be due to its inclination.
