The galaxy presents a generally smooth, elliptical morphology. It appears largely spheroidal, with a high degree of central concentration in luminosity. There is a distinct lack of any apparent spiral arm structure or significant dust lanes. Color gradients suggest the presence of an older stellar population. The central region exhibits a yellowish hue, potentially indicating a population of evolved stars, while the outer regions appear slightly bluer, suggesting some ongoing, but low-level, star formation. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a recent major merger event, though minor disturbances cannot be ruled out. The object's moderate redshift indicates a substantial distance. 
