The galaxy presents as a largely featureless, elliptical morphology with a smooth light distribution. The core exhibits a bright, concentrated luminosity, suggesting a high stellar density in the central region. There is a clear radial color gradient, transitioning from a yellowish-white core to a redder halo. The smooth nature of the light distribution indicates a lack of significant ongoing star formation or recent merger events. The galaxy appears relatively isolated, with no obvious tidal features or nearby companion galaxies that would suggest a recent interaction. Based on its overall appearance, it is likely a massive, evolved system with a dominant population of older stars.
