The galaxy presents a largely smooth, elliptical morphology. Its color profile indicates a population of older stars, biased towards the red end of the spectrum. The core exhibits a bright, concentrated luminosity, suggesting a centrally condensed structure, possibly harboring a supermassive black hole. There is no discernible disk component or spiral arm structure visible at this resolution. A slight asymmetry is observed in the outer halo, potentially indicative of minor tidal interactions or past merger events, though the bulk of the galaxy appears undisturbed. The overall form is generally round, deviating only slightly from a perfectly circular shape.
