X-ray red, green, and blue image obtained with XRISM/Resolve and Chandra/ACIS. The red and green channels correspond to the 2.0–5.0 keV and 5.0–10.0 keV bands observed with Resolve, respectively, while the blue channel represents the 2.0–7.0 keV band observed with ACIS, in which the diffuse emission arises from mainly Sgr A East supernova remnant and GCXE. The gold contours show the VLA 4.8 GHz data from the NRAO archive (https://www.vla.nrao.edu/astro/archive/pipeline/position/J174535.6-285839/), indicating the position of Sgr A east supernova remnant with a radio shell of ﹩3\mathop{.}\limits^{^{\prime} }5\times 2\mathop{.}\limits^{^{\prime} }5﹩ (R. D. Ekers et al. 1975). The positions of AX J1745.6−2901 and MAXI J1744−294 are marked. The red and cyan regions indicate the AX J1745.6−2901 and MAXI J1744−294 extraction regions for the spectral analysis.