The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There is a notable lack of spiral arm structures or distinct features indicative of active star formation regions. The light distribution appears relatively uniform, transitioning smoothly from a bright, compact core to a diffuse outer halo. Color gradients are subtle but present, with the central region exhibiting a slightly bluer hue, suggesting the presence of a younger stellar population. The outer regions appear redder, possibly indicating an older, more evolved stellar population. A very subtle asymmetry, perhaps due to minor tidal interactions or dust absorption, is observed. The overall impression is that of a relatively quiescent galaxy.