The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core region exhibits a yellowish hue, suggesting a population of older, redder stars. Moving outwards from the center, the color transitions to a bluer tone, but the overall smooth texture is maintained. There is no discernible spiral arm structure or significant dust lane obscuration. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or ongoing mergers with other galaxies. Its light is relatively redshifted, indicating that it is at a significant cosmological distance. Given the observed characteristics, this galaxy is likely an elliptical galaxy with a considerable stellar mass and a low star formation rate.
