The galaxy presents as a moderately bright, yellowish-orange elliptical galaxy with a fairly smooth texture. It exhibits a high degree of central concentration, with the brightest region located in the core of the galaxy. The isophotes appear mostly regular, suggesting a relatively relaxed morphology. There are some subtle color variations, with the core appearing more yellow, possibly indicating an older stellar population. Fainter, bluer light is detected further from the center, which could indicate more recent star formation in the outer regions. There is no obvious sign of spiral arms, dust lanes, or active galactic nuclei related features within the galaxy's visible structure. Overall, this appears to be a relatively quiescent elliptical galaxy at a significant redshift, indicating a considerable distance from the observer. The estimated size of the galaxy is on the order of a few kiloparsecs. The colors present indicate that this galaxy is dominated by a relatively old stellar population. The absence of significant morphological disturbances suggests that this system is not currently undergoing any major merger events, though some minor disturbances can not be ruled out.
