The galaxy appears to be a relatively smooth, elliptical-like system. The light is centrally concentrated with a radial decrease in surface brightness. There may be a very faint, diffuse halo. There are hints of structure within the central region, though resolution limits detailed morphological classification. Color gradients appear subtle. It is likely a quiescent system, but it is difficult to assess star formation without higher resolution imaging. There is no evidence of strong tidal features, disk-like structures or ongoing merger activity, although a very minor interaction cannot be entirely ruled out. The object appears consistent with a galaxy at a modest cosmological distance.
