The galaxy presents an elliptical morphology with a high degree of central concentration. The light profile appears smooth and relatively featureless. A distinct yellowish-white core is visible, indicating an older stellar population. The outer regions display a bluer hue, though the color gradients are subtle. There is no obvious disk structure or spiral arm patterns. The galaxy shows no evidence of major ongoing mergers or significant tidal disturbances. It possesses an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated.
