The galaxy presents a largely smooth, elliptical morphology. Its color profile suggests an older stellar population, with a yellowish-white core indicative of evolved stars. A subtle reddish halo surrounds the central region, which could signify ongoing, low-level star formation or the presence of dust. The galaxy exhibits a moderate degree of roundness, appearing neither perfectly spherical nor highly elongated. There is no apparent evidence of major mergers or significant tidal disturbances in this image. Overall, the galaxy appears to be a fairly quiescent system.
