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In this paper, we investigate the complexity factor for static cylindrical configuration with anisotropic fluid distribution. We establish field equations, Tolman-Opphenheimer-Volkoff equation, and mass function. We also evaluate structure scalars using orthogonal splitting of the Riemann tensor which leads to the complexity factor. Finally, we deduce some results about stellar objects for vanishing complexity condition.doi:10.1140/epjc/s10052-018-6330-y fatcat:nrdx4ngd3jcfxd2vyd4l2voxtm