  We made a time-resolved photometric campaign of the bright cataclysmic
variable ASAS J071404+7004.3 in 2020. Inight et al. (2022, arXiv/2109.14514)
recently published time-resolved optical spectroscopy, X-ray observations and
long- and short-term optical variations. Although their results were correct in
many parts, they classified ASAS J071404+7004.3 as a VY Scl-type novalike
object. By comparing the ASAS-SN data of this object and the IW And-type object
HO Pup, we showed that their type classification was incorrect. ASAS
J071404+7004.3 showed outbursts from a standstill followed by shallow dips,
which is the defining characteristic of an IW And star. This object
predominantly showed states with low-amplitude dwarf nova-type oscillations,
some of which could be identified as the "heartbeat"-type state as a variety of
the IW And-type phenomenon. The low state described by Inight et al. (2022) was
not a true low state of a VY Scl star, but a dwarf nova-type state with
increased outburst amplitudes. Both ground-based (our campaign) and TESS
observations detected orbital variations whose periods [0.136589(5) d by the
ground-based campaign and 0.1366476(3) d by the TESS data] are in very good
agreement with the one obtained by radial-velocity studies by Inight et al.
(2022). The standstill in 2019-2020 in ASAS J071404+7004.3 was not brighter
than its dwarf nova-type states. The brightest moment of this object occurred
when the amplitudes of dwarf nova-type variations were large, which challenges
the widely accepted interpretation that standstills in Z Cam stars occur when
the mass-transfer rates are high.
