The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The core region exhibits a bright, yellowish hue that gradually diffuses outwards into a less intense, whitish halo. No distinct spiral arms or prominent dust lanes are readily apparent. There may be a minor asymmetry, indicating a possible tidal interaction or minor disturbance, but the overall morphology strongly suggests an evolved system with a significant spheroidal component. The galaxy appears mostly undisturbed with a high degree of roundness. 
