The galaxy presents as an elliptical-like morphology with a smooth light distribution. A color gradient is observed, transitioning from a yellowish core to a bluish outer halo. The structure appears largely spheroidal, exhibiting characteristics suggestive of a relatively evolved system. Evidence of disturbance is visible, with an asymmetry in the outer halo, which may be due to a past merger. The presence of a distinct core suggests the presence of a supermassive black hole. Star formation is suppressed, with indications of a low star formation rate.
