The galaxy appears to be a large, relatively smooth elliptical galaxy. Its morphology is largely featureless, with a centrally concentrated, bright nucleus that gradually fades into a diffuse halo. The galaxy exhibits a slightly elongated shape, with a relatively high degree of roundness but trending towards an elliptical shape. There is no apparent evidence of spiral arm structure or prominent dust lanes. The overall color profile suggests a population of older stars, but with some ongoing star formation; the redder halo and the bluer core indicate this. There is no indication of any major tidal disturbances or ongoing mergers. The light distribution is generally smooth and centrally concentrated.
