The galaxy appears to be a relatively smooth, centrally concentrated system. It presents an elliptical morphology, with a high degree of roundness. There is a noticeable radial color gradient, transitioning from a bright yellowish core to a fainter and slightly bluer outer region. No spiral arms or significant disk-like features are discernible. There is no visual evidence of major mergers or tidal disturbances. The galaxy's light profile suggests a single component system, dominated by an old stellar population, but with some recent star formation occurring in the core.
