This galaxy presents as a centrally concentrated, elliptical system. The core exhibits a bright, yellowish-orange hue, suggesting a population of older stars. The light smoothly diminishes outwards. There is no significant evidence of spiral arm structures or dust lanes within the galaxy, reinforcing its elliptical classification. The galaxy appears relatively undisturbed, with no noticeable signs of recent mergers or major tidal interactions. Its shape is predominantly round. The galaxy possesses a high estimated mass and, judging from its color, a moderate rate of star formation.
