The galaxy exhibits a generally smooth morphology, appearing largely spheroidal. The central region displays a concentrated, bright yellowish-orange hue, suggesting an older stellar population or significant dust obscuration. A fainter, more diffuse greenish-blue halo surrounds the central region, which could indicate the presence of younger, hotter stars, albeit at a lower overall star formation rate. There is some subtle evidence of possible minor disturbance or tidal features. The galaxy appears relatively isolated, with no obvious major mergers or interacting companions visible in the immediate vicinity. Overall, it appears to be a massive galaxy.
