Left: true color image constructed from the MUSE data using the g, r, and i filters of Megacam at CFHT as colors. The locations of the detected PNe are shown with blue circles. In green, we show the detected GCs. GCs 4, 5, and 6 were part of the L17 sample: their number in that catalog is given after their name. The two red circles show detections that were classified by L17 as GC candidates but are not confirmed with the present data. Right: zoom-out true-color image from CFHT (g, r, i bands from Duc et al. 2015). The MUSE and SKY pointings are shown, respectively, in white and yellow. The SAURON pointing from de Zeeuw et al. (2002) is shown in blue. The MUSE and SAURON pointings are, respectively, 1′×1′ and 33″ × 41″ wide. Assuming a distance to NGC 474 of 30.9 Mpc (Cappellari et al. 2011), 1′ encompasses around 8.9 kpc. North is up and west is right.