We report the first simultaneous X-ray spectropolarimetric observation of the bright atoll neutron star low-mass X-ray binary performed by the Imaging X-ray Polarimetry Explorer ( joint with and The source does not exhibit significant polarization in the 2--8 keV energy band, with an upper limit of 1.3<!PCT!> at a 99<!PCT!> confidence level on the polarization degree. The observed spectra can be well described by a combination of thermal disk emission, the hard Comptonization component, and reflected photons off the accretion disk. In particular, from the broad Fe Kalpha line profile, we were able to determine the inclination of the system ($i which is crucial for comparing the observed polarization with theoretical models. Both the spectral and polarization properties of are consistent with those of other atoll sources observed by Therefore, we may expect a similar geometrical configuration for the accreting system and the hot Comptonizing region. The low polarization is also consistent with the low inclination of the system.