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In this work we obtain an analytic and well behaved solution to Einstein'sfield equations describing anisotropic matter distribution. It's achieved inthe embedding class one spacetime framework using Karmarkar's condition. Weansatz the metric potential $g_{tt}$ corresponding to Wyman IIa solution. Theobtained model is representing some strange star candidates such as Cen X-3,LMC X-4 and 4U 1538-52. A graphical analysis shows that our model is free fromphysical and geometric singularities and satisfies all the physicaladmissibility conditions from the physical and mathematical point of view.

Anisotropic fluid spheres satisfying Karmarkar condition