The galaxy appears as a moderately bright, elliptical-shaped object with a smooth, diffused light profile. Its core exhibits a concentrated, yellowish hue, suggesting a high density of older stellar populations. Fainter, greenish-blue hues are observed in the outer regions, hinting at the presence of some ongoing, albeit limited, star formation. The overall structure indicates a likely lack of spiral arms or significant disk features. The galaxy's shape shows some elongation, resembling a cigar shape, but is still somewhat close to circular. There are no obvious signs of major disturbances or interactions with other galaxies, although minor irregularities in its outer regions are visible. The light emitted indicates that the object is at a considerable distance with a moderate redshift.
