We studied the dependence of selected structural and kinematic properties of early-type galaxies (ETGs) on their environments. The selected sample, extracted from the SDSS-DR17 MaNGA survey, consists of 946 ETGs in clusters (cETGs) and 288 isolated ETGs (iETGs) within a spectroscopic redshift $z\leq 0.15$ . We investigated the distribution of these galaxies in the Fundamental Plane (FP), Kormendy Relation (KR), Faber-Jackson Relation (FJR) and the Mass-Size Relation (MSR). We found that massive galaxies, whose stellar masses $M_{*}> 10^{11}M_{\odot }$ , are predominantly elliptical ( $>65\%$ ). The analysis of the four scaling relations showed that the effect of the host environment is negligible for massive ( $M_{*}>10^{11.5}M_{\odot }$ ) ETGs, most likely because of their passive evolution through dry mergers and/or stellar aging. On the other hand, low-mass ETGs are influenced by their environment, where iETGs with $M_{*}<10^{10}M_{\odot }$ and velocity dispersion $\sigma _{0}\leq 100$ km/sec are $25\%$ more luminous and $11.5\%$ larger than cETGs. Low-mass cETGs may have suffered processes that removed their gas content and hence quenched star formation while low-mass iETGs may have experienced a recent wet merger that triggered star formation and led to their, currently, observed low mass-to-light ratio. However, further spectral analysis is needed to confirm these findings.
