From the cosmological parameters paper of the Planck collaboration:
"If we accept that the base CDM model
is the correct cosmology, then as discussed in Sect. 5 Planck is
in tension with direct measurements of the Hubble constant (at
about the 2,5 sigma level) and in mild tension with the SNLS Type
Ia supernova compilation (at about the 2 sigma level). For the base
CDM model, we also find a high amplitude for the present-day
matter fluctuations, σ8 = 0,828±0,012, in agreement with previous
CMB experiments. This value is higher than that inferred
from counts of rich clusters of galaxies, including our own analysis
of Planck cluster counts (Planck Collaboration XX 2013).
One possible interpretation of these tensions is that some
sources of systematic error are not completely understood in
some astrophysical measurements. The fact that the Planck results
for the base CDM model are in such good agreement with
BAO data, which are based on a simple geometrical measurement,
lends support to this view. An alternative explanation is
that the base CDM model is incorrect.
Our overall conclusion is that the Planck data are remarkably
consistent with the predictions of the base CDM cosmology.
However, the mismatch with the temperature spectrum at
low multipoles, evident in Figs. 1 and 39, and the existence of
other “anomalies” at low multipoles, is possibly indicative that
the model is incomplete. The results presented here are based on
a first, and relatively conservative, analysis of the Planck data.
The 2014 data release will use data obtained over the full mission
lifetime of Planck, including polarization data. It remains
to be seen whether these data, together with new astrophysical
data sets and CMB polarization measurements, will offer any
convincing evidence for new physics."
I think saying "it is possibly indicative that the model is incomplete" is at the least an understatement, but it is also understandable given where is coming from.