The galaxy presents as a relatively smooth, lenticular or early-type spiral galaxy with a slight central bulge and a faint, diffuse disk component. The overall shape is in between round and elliptical. There is very little, if any, apparent substructure within the disk, such as spiral arms or dust lanes. There is no evidence of a strong bar structure. Color gradients suggest an aging stellar population and a lower rate of ongoing star formation, with a somewhat redder hue in the central regions and slightly bluer hues toward the outskirts of the disk. The galaxy appears isolated, with no clear signs of tidal interactions or major disturbances indicating recent mergers. There is a possibility of a minor merging event occuring.
