A significant percentage of galaxies are believed to harbor supermassive black holes (SMBHs) at their centers, although the exact percentage remains uncertain due to limited observations of the universe. The discussion highlights the possibility that some ancient galaxies, formed shortly after the universe's inception, may not contain SMBHs, with direct collapse black holes being a potential formation mechanism. Research suggests that SMBHs could form rapidly in the early universe, influencing galaxy formation. Several academic papers were shared to explore the concept of direct collapse black holes further. Overall, the consensus leans toward a high prevalence of SMBHs in massive galaxies.