The galaxy appears to be a relatively smooth, elliptical galaxy, potentially at intermediate redshift. It presents a largely featureless morphology, with a high degree of central concentration. The galaxy exhibits a yellow-orange hue that transitions into a greenish-yellow halo, indicative of a dominant population of older stars. The round shape suggests minimal rotational support. There's a hint of a possible minor disturbance in the surrounding halo. Overall, the light distribution indicates a galaxy with limited ongoing star formation.
