A supermassive black hole is an astronomical object with an immense gravitational pull, characterized by a mass ranging from millions to billions of times the mass of the Sun. These structures are found at the gravitational centers of most large galaxies, playing a critical role in the overall dynamics and evolution of their host galaxies. The gravitational influence of such an object dictates the orbital paths of surrounding stars and gas. While not directly visible, their presence is inferred through the observable effects of extreme stellar motions and surrounding superheated matter spiraling into the region, forming an accretion disk. The boundary of no return for matter falling into the singularity is known as the event horizon.