  In this work, predictions of the Ginzburg-Landau theory of dark energy (GLT)
for CMB lensing are studied. We find that the time and scale dependence of the
dark energy fluctuations in this semi-phenomenological model is favored by data
in several ways. Firstly, unlike $\Lambda$CDM, $\ell\leq801$ and $\ell>801$
ranges of the CMB angular power spectrum are consistent in this framework.
Secondly, the lensing amplitude $A_L$ is completely consistent with unity when
GLT is confronted with CMB data, even without including CMB lensing data.
Therefore lensing anomaly is absent in this model. Furthermore, the background
evolution of dark energy in this model is able to reconcile the $H_0$ inferred
from CMB with that of directly measured through observing nearby standard
candles.
