To determine the mass of an Active Galactic Nucleus (AGN) from a given luminosity of 12 trillion solar luminosities, one cannot rely solely on the mass-luminosity relationship applicable to main sequence stars. Instead, integrating the luminosity over the galaxy's angular size is necessary, though this method is complex and not commonly used due to the availability of simpler estimation techniques. Knowing the distribution of stars within the galaxy can help, particularly if they are assumed to be main sequence stars, allowing for an integration that normalizes to the total luminosity. This approach typically reveals a linear relationship between luminosity and mass, with a proportionality constant ranging from 1 to 10. However, the presence of an active central engine complicates the calculations significantly.