We report on the second observing program of the active galactic nucleus NGC 4151 with simultaneous Imaging X-ray Polarimetry Explorer (IXPE; 750 ks) (sim 60 ks) XMM-Newton (sim 75 ks), and NICER (sim 65 ks) pointings. NGC 4151 is the first Type-1 radio-quiet Seyfert galaxy with constrained polarization properties for the X-ray corona. Despite the lower flux state in which the source was re-observed and the resulting higher contribution of the constant reflection component in the energy band, our results are in agreement with the first detection. From polarimetric analysis, a polarization degree Pi = 4.7 pm 1.3<!PCT!> and polarization angle Psi = 77 pm 8 east of north (68<!PCT!> c.l.) were derived in the 2.0 -- 8.0 keV energy range. Combining the two observations leads to polarization properties that are more constrained than those of the individual detections, showing Pi = 4.5 pm 0.9<!PCT!> and Psi = 81 pm 6 (with a detection significance of sim 4.6sigma ). The observed polarization angle aligns very well with the radio emission in this source, supporting, together with the significant polarization degree, a slab or wedge geometry for the X-ray corona. However, a switch in the polarization angle at low energies ($37 in the 2-3.5 keV bin) suggests the presence of another component. When it is included in the spectro-polarimetric fit, a high polarization degree disfavors an interpretation in terms of a leakage through the absorbers, instead pointing to scattering from some kind of mirror.
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