The galaxy appears as a centrally concentrated, ellipsoidal object with a smooth, diffuse profile. Its core exhibits a bright, concentrated intensity, suggesting a high stellar density. Moving outward from the center, the luminosity gradually decreases, indicating a declining stellar population density. The overall color of the galaxy seems to be dominated by older stellar populations, with a yellowish-white hue, though there is subtle blueish light present. The edges of the galaxy are not sharply defined but rather blend softly into the background sky, further emphasizing the smoothness of its structure. There are no visible spiral arms, bars, or dust lanes discernible in the image at this resolution, hinting at an early-type morphology. The galaxy is not perfectly spherical, displaying a slight flattening along one axis. No signs of ongoing major mergers or significant tidal disturbances are apparent, suggesting that it has likely undergone a relatively quiescent evolutionary history.
