The galaxy presents as a single, relatively smooth object with a concentrated core. The light is primarily emitted in the redder wavelengths. It appears mostly spheroidal in shape with hints of being slightly oblong. There is a subtle, extended halo surrounding the central region. The smoothness of the light distribution implies a lack of significant spiral arm structure or intense star forming regions. There is an apparent neighboring galaxy close by that is similar in size and color. There is no clear morphological evidence of major tidal disturbances or ongoing mergers.
