A radio galaxy is an astronomical source characterized by powerful radio emissions originating from the centers of galaxies. These emissions are typically associated with active galactic nuclei, where immensely powerful jets of plasma are ejected from a supermassive object at the galactic core. These jets interact with the surrounding intergalactic medium, creating large, elongated structures known as lobes. The morphology and intensity of the radio emission provide crucial observational data about the processes powering the central object, including the mechanisms of particle acceleration and the dynamics of magnetic fields on cosmological scales.