The galaxy appears as a centrally concentrated object with a smooth, diffuse halo. There is an apparent lack of spiral arm structure or a distinct disk component. The color profile suggests a relatively uniform stellar population, leaning toward older stars given the reddish hues observed in the outer regions. The morphology suggests an elliptical galaxy. There is no obvious ongoing major merger activity or strong tidal features, although there is a hint of minor disturbance to the morphology. The overall form is consistent with a galaxy undergoing little to no star formation.
