The galaxy presents as a relatively compact and luminous object. Its overall color appears to be a slightly blueish-white, suggesting a moderate population of young, hot stars. The morphology seems generally smooth and elliptical, with a high degree of central concentration. There is no evidence of a strong spiral structure or distinct features such as prominent dust lanes. Indications point toward little to no ongoing star formation, which fits with the smooth, elliptical morphology. The light emitted indicates it is a massive galaxy. There is no strong evidence of an ongoing merger. It is a fairly round galaxy.
