The galaxy presents as a roughly elliptical object with a smooth, centrally concentrated light distribution. The core exhibits a brighter, more intense blue-white luminosity, with a surrounding halo that gradually fades in intensity. The isophotes appear elongated, exhibiting a disc-like morphology. There is some asymmetry in the outer regions with a possibility of a minor disturbance, possibly suggestive of a past or ongoing minor interaction or merger. The galaxy exhibits a red shift placing it at a considerable cosmological distance, and suggesting its light has been affected by cosmological expansion. The galaxy possesses colors characteristic of evolved stellar populations.
