The galaxy presents as an elliptical, spheroid structure with a smooth and diffuse light distribution. The color profile indicates a population of older stars with a dominant reddish hue. The galaxy appears relatively undisturbed, showing no major signs of tidal interactions or ongoing mergers. There is no presence of obvious features like spiral arms or a prominent central bar. The central region exhibits a slightly higher concentration of light, suggesting the presence of a galactic nucleus. No distinct dust lanes or patches of star formation are immediately apparent. The overall morphology suggests a passively evolving system.
