We report on new VLA radio and XMM-Newton X-ray observations of the SNR G352.7-0.1 .
These high sensitivity , high resolution data reveal that G352.7-0.1 belongs to the thermal composite morphological class .
Small scale structures in radio and X-ray emission are not always correlated and are different for the different X-rays bands examined .
The distance to G352.7-0.1 can be constrained between 6.6 and 8.4 kpc .
The study of the HI suggests that G352.7-0.1 is located within a cavity probably created by the stellar wind of the precursor star .