ABSTRACT: Images of Sgr A West at 8.7 micron , 12.5 micron , 20.8 micron and 24.5 micron were taken on 13 and 15 March 1998, and 15 June 1998 at the Keck 10m telescope with the mid-infrared camera MIRLIN. MIRLIN uses a 128 X 128 Si:As BIB (hi-flux) detector with a scale at Keck of 0.138 ''/pixel. The images are diffraction limited at 24.5 micron and near diffraction limited at 8.7 micron with the seeing FWHM~0.15'' at 8.7 micron . The images will be presented and a limit on the flux at the position of Sgr A* will be calculated at all wavelengths. In addition, the images will be used to investigate the color temperature and dust density distribution within the field.