The galaxy presents as a centrally concentrated, ellipsoidal structure. A dominant, smooth, yellowish-white luminosity emanates from the core region, gradually fading into a less intense, bluish halo. The overall morphology suggests a relatively evolved system, potentially an elliptical galaxy or a lenticular galaxy seen close to edge-on. There are subtle indications of a flattened disk-like structure. The absence of well-defined spiral arms or significant dust lanes points towards a galaxy with a suppressed rate of active star formation. Faint hints of disturbance might be present, although a major ongoing merger is unlikely, as evidenced by the relatively undisturbed form. The distribution of light appears mostly uniform, indicating an older stellar population.
