  We investigate the tidal forces exerted by a spherically symmetric static
parametrized black hole. Our analysis reveals that the radial and angular
components of the tidal forces exerted by the black hole can exhibit both
positive and negative values near the black hole, depending on matters of the
spacetime parameters. Unlike the scenario with the Schwarzschild black hole,
where the radial tidal force (angular tidal force) is always stretching
(compressing) and becomes infinite at the center of the spacetime, the
parametrized black hole allows for finite and compressing (stretching) forces
within the event horizon. Additionally, we derive the geodesic deviation
equations for a particle in free fall and proceed to solve them through
numerical methods. Our analysis demonstrates that the spacetime parameters
$\epsilon$ and $a_1$ exhibit contrasting influences on the magnitudes of the
physical quantities associated with tidal effects.
