The galaxy appears as a centrally concentrated, elliptical object. The core exhibits a reddish hue, transitioning outwards to a yellowish-white halo with traces of green. The light distribution suggests a smooth profile, with no obvious spiral arm structures or prominent dust lanes. The overall shape approximates a circular morphology. There are no obvious signs of tidal disturbances or ongoing mergers. The color gradient from red in the center to a lighter color in the outskirts indicates a possible radial change in stellar population, with older stars potentially dominating the core region and a presence of younger stars further out.
