The galaxy presents as a roughly circular, fairly smooth structure with a bright, concentrated central region. The core exhibits an orange hue, suggesting a population of older stars or significant dust obscuration. Fainter, more diffuse material surrounds the bright core, displaying a gradual transition in color towards the edges. The outer regions appear somewhat greenish, potentially indicating a population of younger, hotter stars or ongoing star formation. There is no evidence of spiral arms or a distinct disk structure. The overall morphology suggests an elliptical galaxy, although the faint greenish outer regions could indicate recent, minor interactions or accretion events. There is no obvious evidence of major mergers or tidal disturbances.
