The galaxy presents as a relatively smooth, elliptical or lenticular structure. There is a central concentration of light, suggesting a well-defined nucleus or bulge. The overall color appears slightly yellow or reddish, indicating an older stellar population with fewer young, massive stars. There is a lack of distinct spiral arms or dust lanes, supporting the classification as an early-type galaxy. The light distribution seems fairly uniform and without significant asymmetries, meaning there are no obvious signs of a recent major merger or tidal disturbances. It is likely that this galaxy has had a significant amount of its star formation quenched.