The galaxy presents a relatively smooth, elliptical morphology. The central region exhibits a high concentration of light, indicative of a prominent galactic nucleus or bulge. A color gradient is observed, with the core appearing slightly redder, possibly suggesting an older stellar population or dust obscuration. Moving outwards, the halo becomes less concentrated and transitions towards bluer hues, which could indicate the presence of younger stars and ongoing star formation activity. The overall structure suggests a galaxy that is evolving, but is fairly undisturbed at the present moment. There is a small possibility of minor distortions in the outer halo.
