The galaxy presents as a generally smooth, elliptical or lenticular structure. A prominent central bulge dominates the morphology, exhibiting a concentrated and bright yellowish-white hue, which indicates a population of older stars. The galaxy displays a high degree of central concentration with a gradual decrease in luminosity moving outward from the core. There may be subtle faint extensions or tidal features, but the overall impression is that of a relatively relaxed and undisturbed system. The primary light distribution appears largely smooth, with minimal evidence of distinct spiral arms or significant star formation regions. The shape is somewhere between round and elongated. 
