The galaxy presents as a largely featureless elliptical morphology. It exhibits a smooth, concentrated light profile with a high degree of central concentration. The observed color is slightly redder in the core, transitioning to a marginally bluer hue in the outer regions of the galaxy. There is no evidence of spiral arms, bars, or any significant dust lanes. The galaxy appears relatively undisturbed, lacking any tidal features or signs of recent mergers. Based on these characteristics, this galaxy is likely a passively evolving system with a minimal star formation rate and a high stellar mass.
