The galaxy appears as a centrally concentrated, relatively smooth object. The overall color profile leans towards yellowish-white, suggesting a population of older stars. There is no discernible spiral structure or distinct disk component visible. The object exhibits a high degree of circularity, with a smooth, gradual decline in luminosity from the core outwards. No signs of tidal disturbances or ongoing merger activity are apparent. Based on the light profile and lack of features, the galaxy is likely an elliptical type, consistent with a quiescent star formation history.
