The galaxy appears to be an elliptical galaxy, elongated in shape with a high degree of central concentration. The light profile suggests it is a relatively smooth system, lacking significant distinct features like spiral arms. The color gradient indicates a higher concentration of older stars or dust towards the center, giving the core a yellowish to orange hue. The outer regions show a subtle blueish tint. A minor perturbation cannot be ruled out due to the faint light around the center, but the galaxy appears mostly undisturbed. There is no definitive sign of an ongoing major merger, and the overall structure suggests a lack of significant recent star formation or tidal interactions.
