Pseudo-RGB images constructed from the combined MUSE datacube before (top) and after (bottom) removing the stellar and nebular continuum in each spaxel, with the R, G, and B channels corresponding to the summed 6900 Å → 7100 Å, 4900 Å → 5100 Å, and 5300 Å → 5500 Å (observed) spectral ranges, respectively. The intensity stretch of each channel differs between both images for greater clarity. Stars appear in hues of blue and red, whereas the O-rich fast-moving ejecta are visible as bright green filaments.