  We numerically investigate the evolution of the holographic subregion
complexity during a quench process in Einstein-Born-Infeld theory. Based on the
subregion CV conjecture, we argue that the subregion complexity can be treated
as a probe to explore the interior of the black hole. The effects of the
nonlinear parameter and the charge on the evolution of the holographic
subregion complexity are also investigated. When the charge is sufficiently
large, it not only changes the evolution pattern of the subregion complexity,
but also washes out the second stage featured by linear growth.
