The galaxy appears as a centrally concentrated, smooth elliptical. There is a distinct lack of resolved spiral arms or prominent dust lanes. The light profile decreases steadily from the core outwards, suggesting a relatively uniform stellar population. Color gradients are subtle, with a slightly bluer hue towards the outer regions, possibly indicating younger stars at the edges. The overall shape is nearly spherical with only a slight ellipticity. There are no signs of major tidal disturbances or ongoing mergers. The galaxy appears to be a quiescent system.
