The galaxy presents as a centrally concentrated system, exhibiting a smooth, largely featureless morphology. The core region displays a distinct yellowish-orange hue, which transitions outwards to a more diffuse greenish halo. The overall shape of the galaxy appears mostly rounded, with only the faintest hint of ellipticity. There is no readily apparent evidence of spiral arms or other disk-like structures. Close inspection reveals no signs of major ongoing mergers or significant tidal disturbances, though subtle asymmetries could indicate minor interactions. The galaxy's color profile suggests a relatively quiescent stellar population, with the central bulge possibly dominated by older, redder stars and the outer regions showing slightly bluer colors, indicative of more recent, albeit subdued, star formation activity.
