  The Hubble tension resides in a statistically significant discrepancy between
early time and late time determinations of the Hubble constant. We discuss the
Hubble tension within the Ellipsoidal Universe cosmological model. We suggest
that allowing small anisotropies in the large-scale spatial geometry could
alleviate the tension. We, also, show that the discrepancy in the measurements
of the Hubble constant is reduced to a statistically acceptable level if we
assume sizeable cosmological anisotropies during the Dark Age. In addition, we
argue that the Ellipsoidal Universe cosmological model should resolve the $S_8$
tension.
