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We report on XMM-Newton and Chandra observations of the Galactic supernovaremnant candidate G38.7-1.4, together with complementary radio, infrared, andgamma-ray data. An approximately elliptical X-ray structure is found to be wellcorrelated with radio shell as seen by the Very Large Array. The X-ray spectrumof G38.7-1.4 can be well-described by an absorbed collisional ionizationequilibrium plasma model, which suggests the plasma is shock heated. Based onthe morphology and the spectral behaviour, we suggest that G38.7-1.4 is indeeda supernova remnant belongs to a mix-morphology category.

Identification campaign of supernova remnant candidates in the Milky Way. II. X-ray studies of G38.7-1.4