Possible scaling relations of (a) stellar-to-gas mass ratio versus gas mass (log₁₀M_*/M_gas vs. log₁₀M_gas), (b) stellar-to-gas mass ratio versus total dynamical mass (log₁₀M_*/M_gas vs. log₁₀M_dyn), and (c) total baryonic mass versus total dynamical mass (log₁₀M_b vs. log₁₀M_dyn). The UDGs, LSBs, HSBs, and the dwarfs are shown in teal, yellow, blue, and magenta colours, respectively. Each of the galaxy samples are divided into two sub-samples – isolated (denoted with filled circles) and tidally bound (denoted with empty circles). The scaling relations are obtained for the two sub-samples of each galaxy classes separately and plotted with solid and dashed lines, respectively.