NGC 1275 is a prominent galaxy located in the constellation Perseus. It is classified as a type of active galaxy known as a blazar, which emits powerful jets of energy. NGC 1275 is part of the Perseus Cluster, one of the nearest and most studied galaxy clusters. This galaxy is notable for its bright central region, which contains a supermassive black hole. The intense gravitational forces around this black hole lead to the emission of high-energy radiation, making NGC 1275 a key object of study in astrophysics. Its distance from Earth is approximately 250 million light-years.