The ubiquity of substructures such as gaps and rings around Class II disks suggests that planet formation might have already started during the embedded stages of protostellar evolution. To address how and when planet formation might begin, the Atacama Large Milimeter/submilimeter Array (ALMA) large program Early Planet Formation in Embedded Disks (eDisk) target a sample of 19 deeply embedded protostars in nearby star-forming regions with high angular resolution dust continuum and line observations. In this poster, we present the first results from eDisk, with particular focus on the Class 0 protostars BHR71 IRS1/2 and RCrA IRS5N. The 1.3 mm continuum emissions from all three sources are smooth and show no substructures. However, brightness asymmetries are observed along the minor axis for all sources, suggesting the disks are optically thick, possibly reflecting early grain growth. The gas kinematics traced by observations of C18O make it possible to distinguish between the infalling gas and Keplerian rotating disks toward the sources and thus trace the physical and chemical evolution of material delivered to the protoplanetary disks in their earliest stages.