The galaxy appears as a somewhat symmetrical elliptical or lenticular type. Its light distribution suggests it is relatively smooth, with a high concentration of light towards the center. The main body of the galaxy displays a centrally concentrated bulge or core, surrounded by a diffuse halo. The morphology suggests it is relatively undisturbed, lacking strong tidal features or evidence of a recent major merger, though there are some possible signs of minor disturbances. The galaxy's color indicates a population of older stars, emitting more light in the redder part of the spectrum. It displays a general roundness with a mild elongation. Its size is relatively compact.
