The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. It is roughly circular in shape, displaying a high degree of radial symmetry. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region. The light smoothly decreases away from the center, implying a lack of significant spiral arm structures or dust lanes. There are no obvious signs of recent merger activity or major tidal disturbances. Subtle irregularities in the outer regions hint at possible minor interactions, but overall the galaxy appears relatively undisturbed.
