  In this paper we will construct a linearized metric solution for an
electrically charged system in a {\it ghost-free} infinite derivative theory of
gravity which is valid in the entire region of spacetime. We will show that the
gravitational potential for a point-charge with mass $m$ is non-singular, the
Kretschmann scalar is finite, and the metric approaches conformal-flatness in
the ultraviolet regime where the non-local gravitational interaction becomes
important. We will show that the metric potentials are bounded below one as
long as two conditions involving the mass and the electric charge are
satisfied. Furthermore, we will argue that the cosmic censorship conjecture is
not required in this case. Unlike in the case of Reissner-Nordstr\"om in
general relativity, where $|Q|\leq m/M_p$ has to be always satisfied, in {\it
ghost-free} infinite derivative gravity $|Q|>m/M_p$ is also allowed, such as
for an electron.
