Examples of Perseus cluster dwarf galaxies with more than ten GCs (N_GC > 10) in I_E data. The majority of such dwarf galaxies have a stellar mass of M_* > 10⁸ M_⊙, while they cover a range of central surface brightness (μ₀) and effective radius (R_e). The Euclid ID of dwarf galaxies from Marleau et al. 2025 are written on top of each cutouts, as well as their name in Janssens et al. 2022 when available (written in parenthesis). The cutouts have dimensions of 40″ × 40″ (about 14 × 14 kpc).