This galaxy appears to be a relatively smooth, elliptical or lenticular system. It has a centrally concentrated luminosity profile, with a gradual falloff in surface brightness toward its periphery. The color indices suggest a relatively evolved stellar population. No prominent dust lanes or spiral arm features are discernible in the available image. There is no evidence of a major ongoing merger, though minor tidal disturbances cannot be ruled out. The overall morphology indicates it is a fairly regular, undisturbed system.
