  Coronal loops serve as the fundamental building blocks of the solar corona.
Therefore, comprehending their properties is essential in unraveling the
dynamics of the Sun's upper atmosphere. In this study, we conduct a comparative
analysis of the morphology and dynamics of a coronal loop observed from two
different spacecraft: the High Resolution Imager (HRI$_{EUV}$) of the Extreme
Ultraviolet Imager aboard the Solar Orbiter and the Atmospheric Imaging
Assembly (AIA) aboard the Solar Dynamics Observatory. These spacecraft were
separated by 43$^{\circ}$ during this observation. The main findings of this
study are: (1) The observed loop exhibits similar widths in both the
HRI$_{EUV}$ and AIA data, suggesting that the cross-sectional shape of the loop
is circular; (2) The loop maintains a uniform width along its entire length,
supporting the notion that coronal loops do not exhibit expansion; (3) Notably,
the loop undergoes unconventional dynamics, including thread separation and
abrupt downward movement. Intriguingly, these dynamic features also appear
similar in data from both spacecraft. Although based on observation of a single
loop, these results raise questions about the validity of the coronal veil
hypothesis and underscore the intricate and diverse nature of complexity within
coronal loops.
