The galaxy presents as a centrally concentrated spheroid with a relatively smooth morphology. The luminosity profile appears to be fairly regular, without substantial tidal features or asymmetries suggestive of recent major mergers. The color is generally yellow, with a slight reddening toward the core of the galaxy. The overall appearance suggests a potentially evolved system with a relatively quiescent star formation rate. There are subtle hints of a flattened, disk-like structure, but the spheroid component dominates the galaxy's light distribution.
