Understanding how star formation proceeds in dwarf galaxies across diverse environments is essential for constraining the physical processes that regulate baryon cycles and govern the evolutionary pathways of low-mass systems. In this study, we use high-resolution JWST/NIRCam and archival HST imaging to perform a spatially resolved (to a physical resolution of ∼250 pc) investigation for three dwarf galaxies at z ≈ 0.08 selected from the Cosmic Evolution Early Release Science Survey (CEERS) in the Extended Groth Strip field. Despite comparable stellar masses, the three galaxies exhibit distinct internal star formation morphologies. CEERS-31176 shows a localized, asymmetric star formation offset from a smooth old stellar component. CEERS-60352 hosts a compact star formation core embedded in an older structure, with a V-shaped specific star formation rate profile and a bimodal resolved star formation main sequence. CEERS-81077 is dominated by clumpy star formation, including a prominent off-nuclear clump decoupled from the stellar mass distribution. Their spatially resolved star formation main sequence slopes span α = 0.26–1.61, reflecting diverse regimes of star formation regulation. These case studies highlight the role of both external accretion and internal feedback as plausible regulators of star formation in dwarf galaxies out of the Local Volume.