The galaxy appears to be a relatively smooth, elliptical-type galaxy. Its morphology is largely spheroidal with no apparent spiral arm structure. It has a concentrated central bulge that is yellowish-white, suggesting a population of older stars. The color becomes slightly redder towards the outer regions, which further suggests an aging stellar population with diminished ongoing star formation. There is no apparent dust lane or significant morphological disturbance indicating any recent major merger events. The galaxy appears isolated and undisturbed. Overall, the morphology indicates a well-evolved, relatively quiescent system.
