Best-fit SED and cutouts for our source. Left: multi-component template STARDUST spectrum (grey line and shaded areas), the observed photometry (red squares), including the upper limits (red arrows) are also displayed. Radio measurements from VLA at 1.4 (Schinnerer et al. 2010) and 3 GHz (Smolčić et al. 2017) are overlaid in blue. The SED is separated into three components – stellar emission (blue), AGN emission (green), dust (red). Right: optical-NIR-FIR cutouts of our galaxy, ranging from 5″.0 in the optical-MIR range to 50″.0 in FIR.