  We report new total intensity visible light high contrast imaging of the TW
Hya disk taken with the Space Telescope Imaging Spectrograph (STIS) on the
Hubble Space Telescope (HST). This represents the first published images of the
disk with STIS since 2016, when a moving shadow on the disk surface was
reported. We continue to see the shadow moving in a counter-clockwise fashion,
but in these new images the shadow has evolved into two separate shadows,
implying a change in behavior for the occulting structure. Based on radiative
transfer models of optically thick disk structures casting shadows, we infer
that a plausible explanation for the change is that there are now two
misaligned components of the inner disk. The first of these disks is located
between 5-6au with an inclination of 5.5\arcdeg and PA of 170\arcdeg, the
second between 6-7au with and inclination of 7\arcdeg and PA of 50\arcdeg.
Finally, we speculate on the implications of the new shadow structure and
determine that additional observations are needed to disentangle the nature of
TW Hya's inner disk architecture.
