The galaxy presents as a luminous, elliptical structure with a smooth, concentrated morphology. The central region exhibits a bright, yellowish core, indicative of a high density of older stellar populations. The light fades gradually outwards. The surrounding halo appears diffuse and exhibits hints of a reddish hue, possibly indicating the presence of evolved stars or dust. The overall shape is slightly elongated but largely spheroidal. There is no apparent spiral arm structure or evidence of significant star formation. There are no signs of tidal disturbances or ongoing merger activity that are readily apparent.
