Supermassive black holes may not form from the merging of stellar black holes due to initial conditions, such as the likelihood of scattering rather than direct collisions. The mass of stellar black holes is significantly lower than that of supermassive black holes, which complicates their merger dynamics. Research suggests that supermassive black holes likely formed through processes involving primordial black holes or the direct collapse of massive first-generation stars. Additionally, the entropy considerations during mergers indicate that the resultant black hole's event horizon must be equal to or greater than the sum of the merging black holes' event horizons. The formation of supermassive black holes remains an active area of research, with various theories attempting to explain their origins.