The galaxy presents as a relatively smooth, elliptical form. Its light profile is concentrated towards the center, with a gradual fading towards the outer regions. The core exhibits a yellowish-white hue, suggesting an older stellar population. There is limited indication of spiral arm structures or significant dust lanes, lending support to its classification as an elliptical galaxy. The galaxy appears fairly isolated and undisturbed with no prominent tidal features or signs of interaction with nearby galaxies. The axial ratio indicates a near-spherical shape.
