This galaxy presents as a relatively compact, elliptical morphology. The light is fairly smooth and centralized, with a dominant yellowish hue. This color suggests an older stellar population with fewer young, hot, blue stars, as opposed to a spiral galaxy with active star formation. No spiral arm structures or dust lanes are apparent. The galaxy appears mostly undisturbed with no major signs of interaction or ongoing merger events. The rounded shape reinforces the suggestion of an elliptical classification.
