  The whole set of INTEGRAL observations of type Ia supernova SN2014J, covering
the period 19-162 days after the explosion has being analyzed. For spectral
fitting the data are split into "early" and "late" periods covering days 19-35
and 50-162, respectively, optimized for $^{56}$Ni and $^{56}$Co lines. As
expected for the early period much of the gamma-ray signal is confined to
energies below $\sim$200 keV, while for the late period it is most strong above
400 keV. In particular, in the late period $^{56}$Co lines at 847 and 1248 keV
are detected at 4.7 and 4.3 $\sigma$ respectively. The lightcurves in several
representative energy bands are calculated for the entire period. The resulting
spectra and lightcurves are compared with a subset of models. We confirm our
previous finding that the gamma-ray data are broadly consistent with the
expectations for canonical 1D models, such as delayed detonation or
deflagration models for a near-Chandrasekhar mass WD. Late optical spectra (day
136 after the explosion) show rather symmetric Co and Fe lines profiles,
suggesting that unless the viewing angle is special, the distribution of
radioactive elements is symmetric in the ejecta.
