The galaxy presents as a flattened, disk-like structure, appearing nearly edge-on from our vantage point. There is a prominent central bulge that is bright and appears largely featureless with a smooth radial light profile, suggestive of an older stellar population. A distinct dust lane is observed, obscuring portions of the disk and indicating the presence of interstellar material. The color of the galaxy exhibits a gradient, with the bulge showing a yellowish-white hue and the disk appearing bluer, implying ongoing star formation in the outer regions. Faint extensions or tidal features are not clearly evident, although there is a slight irregularity in the shape of the disk which may be indicative of minor gravitational interactions. The overall structure points to a spiral or lenticular galaxy, with the observed dust lane suggestive of a spiral nature, though the smooth bulge may point towards an S0 classification. Higher resolution imaging or spectroscopic data would be beneficial to fully characterize the galaxy's type and internal dynamics.
