The galaxy presents as a relatively smooth, elliptical-like structure. The color profile suggests a higher concentration of older stellar populations, with a yellow-red hue dominating the central region, transitioning to a greenish halo further from the core. There appears to be minimal evidence of active star formation, which is consistent with the overall color. The morphology appears largely undisturbed, with no obvious signs of tidal tails, asymmetric features, or a prominent disk. The light is concentrated towards the center. The overall rounded shape suggests a more relaxed, evolved system, with a high likelihood of being classified as an elliptical galaxy.
