The structures of the Somma-Vesuvius volcanic complex are modelled on the basis of the interpretation of gravity anomalies obtained from data available in the literature and acquired along a new profile along the coastline from Naples to Castellammare di Stabia. In order to highlight the contribution of shallow crustal structures, the residual anomalies were considered. A marked gravity low was recognised in the eastern sector of Vesuvius. Furthermore data interpretation was carried out along two profiles centred on the low gravity region in question: a first profile crossing the Vesuvius crater in direction WNW-ESE, and a second one in NNE-SSW direction. The 2 ½ D model obtained reveals a crustal structure characterised by sediments of 2.3 Mg/m3 density, overlying bedrock with a density of 2.6 Mg/m3. Near the volcanic system the model becomes more complex due to the presence of light sediments with a density of 2.1 Mg/m3 overlying a body with a density of 2.4 Mg/m3 which extends into depth. The latter is thought to be closely related to the zone of magma ascent developed along the volcanic axis. Along the coast the volcanic component is reduced and the model shows that the layer with a density of 2.3 Mg/m3 ranges in thickness from 0 to about 3500 m. An additional body between 1500 and 3000 m with a density of 2.4 Mg/m3 was considered in order to account for the slight rise in the residual anomaly in the area in the vicinity of Mt. Vesuvius.