The galaxy presents as an elliptical morphology, with a smooth, featureless appearance. It exhibits a high degree of circularity, showing no discernible elongation or distortion. The color profile suggests an evolved stellar population, dominated by older, redder stars, concentrated towards the center. The galaxy appears to be relatively isolated with no apparent signs of tidal disturbances or ongoing mergers, its structure undisturbed. There is no indication of active star formation regions. The luminosity profile indicates a concentration of light towards the galactic core, fading smoothly towards the outer regions.
