The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge exhibiting a yellowish hue. A fainter, diffused halo surrounds the core, displaying a more subtle greenish tint near the central region, possibly indicating recent or ongoing star formation. There is no clear evidence of spiral arms or a disk-like structure. Minor asymmetrical features or disturbances within the halo suggest a possible interaction or past merger event, though the overall morphology indicates that it is largely undisturbed. The galaxy's color profile suggests a stellar population that is primarily evolved, with possible pockets of younger stars contributing to the subtle greenish regions.
