The galaxy presents an overall elliptical morphology, with a bright, concentrated central core. Moving outwards, a diffuse halo is observed. The color profile is not uniform. The core exhibits a blue-white hue, suggestive of younger, hotter stellar populations. The halo appears more greenish, perhaps indicating older stars or a higher metallicity. A slight asymmetry is noted in the halo's outer regions, possibly indicative of minor gravitational interaction or recent accretion events. Faint, irregular extensions, could be tidal features resulting from past interactions.
