We know that the charged Reissner Nordstr$\"{o}$m black hole metric is obtained from the Einstein Hilbert gravitational action. This action has the kinetic term $F^2 = (da)^2$. Motivated by the higher-form symmetry structure of the EFT of Force Free Electrodynamics, we replace the Maxwell field-strength contribution in the Einstein Hilbert action by the gauge-invariant combination $(b-da)^2$, where $a_\mu$ is the worldsheet gauge field and $b_{\mu\nu}$ is a background two-form field. This ensures that the new action has a higher form symmetry $b \rightarrow b+d\Lambda, a\rightarrow a+\Lambda$. Here, unlike in qed, $\Lambda$ may be any one form (not necessarily a differential one form $\partial_\mu \phi$). The higher form symmetry here is one with the conserved current being a two form and the charge integrated on surfaces. Intuitively, it is the number/current of vector field lines that is conserved here, not the current of particles. Thus, integrating over a surface through which the field lines pierce is sufficient to find the number of these lines that are passing through; so the charge is integrated on surfaces, rather than on the volume. After fixing a particular gauge for the fields $a_\mu$ and $b_{\mu\nu}$, we obtain a generalized black-hole metric. We find that on hypersurfaces satisfying $(r-t)=$ constant, this metric reduces locally to a Reissner Nordstr$\"o$m geometry with an effective charge parameter depending on the constant $(r-t)$.