The galaxy presents as a smooth, elliptical-like object with a high degree of central concentration. The light distribution suggests a bulge-dominated morphology. The galaxy appears yellowish, hinting at an older stellar population with lower star formation rate. There is little to no evidence of spiral arm structure or significant dust lanes. The overall shape indicates an object that is viewed at a slight angle, deviating somewhat from a perfect sphere. There do not appear to be signs of tidal disturbances or ongoing mergers, as the morphology is largely undisturbed.
