The galaxy presents a largely smooth morphology. It appears elliptical in shape, though not perfectly spherical, with a slight elongation. There is a bright, concentrated core that gradually diffuses outward. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region and fainter blue hues on the outer edges. There is no apparent spiral arm structure, or any signs of on-going major mergers. The smooth light distribution and color profile suggest a relatively quiescent galaxy with a stellar mass is somewhere around 10^10.8 solar masses and experiencing some minimal star formation at a rate of roughly 10^0.2 solar masses per year.
