The galaxy presents as a smooth, elongated structure. The central bulge exhibits a concentrated, bright yellowish-orange hue, suggesting a population of older stars. Moving outward from the center, the color transitions to a slightly bluer, less intense shade. This color gradient might indicate a subtle difference in stellar population, with potentially younger stars residing in the outer regions, although star formation appears relatively quiescent. The galaxy's shape is predominantly elliptical, with a hint of a disk-like component, though not sharply defined. There is no evidence of major disturbances or merging activity. The overall appearance implies a galaxy that is relatively evolved, with ongoing but subdued star formation.
