  We investigate the broad line profiles emitted from a system supermassive
binary black hole (SMBBH) having elliptical orbits and low mass ratio of
$m_2/m_1\sim 0.1$. Our model assumes a super Eddington accretion flow in the
case of a smaller component, whereas the massive component has very small or
negligible accretion, therefore supposing that no broad line region (BLR) is
attached to it. Thus, the proposed SMBBH system contains one moving BLR,
associated with the less massive component and one circum-binary BLR. We study
the effect of different total mass of the system (ranging from 10$^6$ to 10$^8$
Solar masses) to the $\mathrm{H\beta}$ line profiles and to the continuum and
line light curves. The resulted broad line profiles are asymmetric and shifted,
and are varying during the orbital period. The asymmetry in the broad line
profiles is discussed in terms of expected differences between the proposed
model of the SMBBH with one active component and the scenario of a recoiling
black hole. We discuss the periodicity detected in the line and continuum light
curves, as well as in the variations of the line asymmetry and shift.
