Density map of the gas structures in the RAMSES simulation for the stellar winds from the WR stars feeding the black hole (Calderón et al. 2025). The gas cells with T < 10⁵ K, inclination −90° < i < 0°, and longitude of ascending node −180° < Ω < 0° are considered to find coherent structures with a similar orientation of the orbital angular momentum to that of X7 and G3. The color bar refers to cell mass. None of the gas cells form any coherent clumps that could evolve into X7.