The galaxy presents as a centrally concentrated elliptical system. It exhibits a smooth, relatively featureless morphology with a discernible but subtle color gradient, trending from a yellowish-white core to slightly bluer outer regions. The overall shape is moderately elliptical, not strongly elongated nor perfectly spherical, with no obvious signs of tidal disturbances or ongoing major merger events. There appears to be a slight asymmetry suggesting a potential minor interaction. The overall color suggests an older stellar population, though the slightly bluer outer regions indicate the presence of some ongoing, albeit modest, star formation.
