  Based on reasonable assumptions, we propose a new expression for Lloyd's
bound, which confines the complexity growth of charged black holes. We then
revisit holographic complexity for charged black branes in the presence of a
finite cutoff. Using the proposed Lloyd's bound we find a relation between the
UV and the behind the horizon cutoff. This is found to be consistent with the
factorization of the partition function at leading order in large N. We argue
that the result may be thought of as a holographic realization of strong cosmic
censorship.
