The galaxy presents a generally smooth and rounded morphology. A concentrated, bright central region dominates the galaxy's appearance. The core exhibits a yellow-orange hue, potentially indicative of an older stellar population or dust obscuration. Surrounding the core, there's a faint, diffuse halo with subtle reddish tinges. The system shows possible signs of disturbance, as the halo appears lopsided. There may be slight evidence of a tidal tail or merger remnant. The overall structure suggests the system may be an elliptical galaxy possibly undergoing some interactions or a minor merger.
