View of a Perseus cluster dwarf galaxy (EDwC-0120 in Marleau et al. 2025, and R84 in Janssens et al. 2024) as seen by the VIS and NISP instruments on board Euclid (in I_E, Y_E, J_E, and H_E) by HST/ACS (in F814W) and by CFHT/MegaCAM (in r). The galaxy seems to host several GCs, which appear as point sources on top of the galaxy, as well as a NSC in the centre of the diffuse component. The brightest object projected near the centre of the galaxy could be a foreground star or a massive GC destined to merge with the already existing NSC.