The theory of Gaussian multiplicative chaos (GMC) is usually defined w.r.t. logcorrelated Gaussian fields in the finite dimensional context and dates back to a seminal work of Kahane [K85] which contains ideas and results that led to a lot of rejuvenated interest in the subject during the last decade. Inspired by ongoing investigations pertinent to the Liouville measure in 2d-Liouville quantum gravity, thick points of the Gaussian free field and volume decay of Liouville balls and scaling exponents, in the present infinite dimensional context we drop all assumptions on log-correlations and consider a centered Gaussian field, driven by space-time white noise and indexed by continuous paths equipped with the law of Brownian paths on R d as reference measure. An exponentiation of this field, followed by suitable renormalization, defines a Gaussian multiplicative chaos on Wiener paths. As long as the coupling constant is tuned sufficiently low (and in this regime it is known that for d ≥ 3, the field attains high values on any path sampled according to the GMC probability measure) and with the white noise field spatially mollified at scale ε > 0, the (renormalized) GMC volume of any microscopic ball of radius ε d/2 in the Wiener space, with its location chosen uniformly therein, decays at least with speed ε d in an almost sure sense as the mollification scheme is turned off. We also show that when the coupling constant is tuned high, the energy landscape of the system freezes and enters the so-called glassy phase as the normalized covariance of the field under the GMC measure concentrates most of its mass in an averaged sense. A key aspect of our proof, while not making any assumptions about log-correlations, builds on Kahane's techniques [K85] in a general set up, combined with geometric properties of the underlying metric space of continuous functions.