The galaxy presents as a centrally concentrated, elliptical-like system. The core region appears smooth and intensely luminous with a reddish hue, indicating a population of older stars and minimal dust obscuration. This central region is surrounded by a more diffuse, greenish halo. This greenish color suggests the presence of some younger stars and potentially ongoing, albeit low-level, star formation or emission from ionized gas. The overall morphology indicates a mature galaxy with minimal signs of recent major mergers or significant tidal disturbances, presenting a relatively undisturbed structure. The galaxy's round shape suggests it does not present with a disk.
