The galaxy presents a generally elliptical morphology, appearing mostly smooth and rounded. The central region exhibits a concentrated, bright core, transitioning outwards to a less luminous, diffuse halo. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region. The outer regions appear bluer, perhaps indicating more recent, though diminished, star formation activity or a population of younger stars. There are no prominent spiral arms or a distinct disk structure visible, and the galaxy shows no obvious signs of major interaction or significant tidal disturbances, although some minor irregularities in the outer regions might suggest minor interactions. The overall appearance is consistent with a relatively massive galaxy.
