The galaxy presents as an elliptical morphology, appearing relatively smooth and featureless. Its color profile indicates a dominant older stellar population, with a central concentration of light suggesting a bulge. The galaxy's shape is generally elongated. There is no obvious evidence of spiral arm structure or significant dust lanes. There is no evidence of major tidal disturbances or recent mergers, although a slight asymmetry is present. The outer regions appear to gradually fade into the background, with no sharp cut-off in luminosity.
