The galaxy presents a smooth, elliptical morphology. Its color profile exhibits a central concentration of yellow-orange hues, suggesting a dominant population of older stars. There is a subtle color gradient, with a slight shift towards redder colors in the outer regions. No spiral arms, prominent dust lanes, or distinct substructures are discernible. The galaxy appears relatively isolated, without significant signs of tidal interaction or ongoing merger activity. The overall light distribution indicates a high degree of symmetry and a well-defined center. The galaxy has a fairly large size and is likely a very massive system with minimal ongoing star formation.
