Tidal forces are most significant feature of geodesic deviation in General Relativity. The astrophysical significance within tidal forces, standpoints out tidal disruption events. We investigate the tidal forces developed in black hole formulated in nonlinear electrodynamic theory. The tidal effects are inversely proportional to the charge in angular and radial direction. The components of tidal obtain by Riemann tensor and geodesic deviation equation. We solve the geodesic deviation equation for radial and angular components of an exact black hole spacetime. Further, we explore the graphical behavior of radial and angular components for different initial conditions.