  Although the existence of asymmetrical profile of [OIII]$\lambda$5007 has
been discovered for ages, its filiation and physics are poorly understood. Two
new spectra of I ZWI taken on Nov 16, 2001 and on Dec 3, 2002 were compared
with the spectra taken by BG92. Following results are obtained. 1)The certain
variations of broad [OIII] during about 10 years separating the observations
are identified. The inferred length scale of broad [OIII] emitting region
ranges from 0.3pc to 3pc. By assuming a Keplerian motion in emitting region,
the material emitting broad [OIII] is likely to be located at transient
emission line region, between BLR and NLR. 2)We find a positive relation
between the FeII emission and flux of H$\beta$(or continuum). On the other
hand, the parameter RFe decreases with ionizing continuum marginally. 3)We
detect a low ionized NLR in I ZWI, because of the low flux ratios
$\rm{[OIII]_{n}/H\beta_{n}}$($\sim1.7$).
