The galaxy presents as a relatively smooth, elliptical or lenticular-like structure, with a notable lack of prominent spiral arms or distinct features. Its overall shape is somewhat elongated, but not extremely so, and it appears quite rounded. There is a very subtle suggestion of some disturbance or minor asymmetry in the outer regions. The galaxy exhibits a color gradient, appearing bluer towards its outer edges and slightly redder towards its central regions, hinting at potential variations in stellar populations or dust content. There are no signs of ongoing major merging activity or significant tidal features.
