As one of the least studied mode waters, the role of the Indian Ocean Subtropical Mode Water (IOSTMW) in influencing the ocean and atmosphere as it is advected in the subsurface remains poorly understood. Taking advantage of the rapid increase of Argo data over the past decade, this study compares the ocean temperature structure during periods of thick and thin IOSTMW. The results indicate notable differences in both temperature and stratification linked to variations in IOSTMW thickness. In terms of temperature, the following phenomena are observed when the IOSTMW is thick: (a) the layer above the IOSTMW experiences colder temperatures, whereas warmer temperatures occur below it; (b) isotherms above the IOSTMW shoal, whereas those below it deepen. As for the stratification, a negative correlation is observed between IOSTMW thickness and stratification at depths between 100 and 300 dbar, suggesting that the presence of thick IOSTMW weakens the stratification within this depth range. Conversely, a positive correlation is observed around 400 dbar, suggesting that thick IOSTMW tends to coincide with a deeper main thermocline. Notably, regions near the Agulhas Current exhibit contrasting characteristics compared to other regions within the study area, indicating the potential impacts of the Agulhas Current meander on ocean temperature structure and the distribution of the IOSTMW. An intriguing question for future studies is how variations in IOSTMW thickness contribute to marine heatwave occurrences and influence atmospheric conditions.