The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The core region exhibits a distinct yellowish hue, suggesting an older stellar population and diminished ongoing star formation. A diffuse, less concentrated halo surrounds the core, displaying a bluer color gradient indicative of younger stars and potential star formation regions. There is a suggestion of faint, spiral-like structures within the outer regions of the galaxy, but they appear ill-defined and disturbed. There is no clear evidence of a major ongoing merger, although a slight asymmetry in the outer regions cannot be ruled out as evidence of a minor past interaction or merger. The overall structure indicates a galaxy that is likely undergoing a transition from a star-forming spiral to a quiescent elliptical type.
