Polarimetric images of the system HD 120326 using VLT/SPHERE at 1.6 μm (broad band H; scattered light; epoch 2018-06-01). We processed the data by using the pipeline IRDAP. From left to right, we show the Stokes vector components pI (intensity), Q_ϕ (azimuthal or radial polarization), and U_ϕ (polarization oriented at ±45° with respect to the azimuth) calibrated in μJy/arcsec², and the signal-to-noise (S/N) map, which is derived on the basis of the Q_ϕ and U_ϕ images. For these images, as all the ones in this paper: north is up and east is left, while the gray circular mask corresponds to the region within the inner working angle of the coronagraph.