The galaxy presents as a centrally concentrated, ellipsoidal structure. The core region exhibits a bright, yellowish hue, suggesting an older stellar population. Moving outwards from the core, the color appears to transition to a more reddish-brown shade, which might be due to the presence of dust lanes. The surface brightness decreases relatively smoothly from the center outwards, with no clear indication of spiral arms or distinct features indicative of recent or ongoing major mergers. The galaxy appears relatively undisturbed, with a high degree of rotational symmetry.
