The galaxy presents a largely smooth and somewhat rounded morphology, exhibiting characteristics indicative of an elliptical galaxy. The object has a diffuse central bulge, with a gradual decrease in luminosity outwards. There is no definitive structure such as spiral arms or a prominent disk observed. There is minimal distortion to the overall structure, but there is evidence of some minor disturbance. The object appears to have a moderate redshift, suggesting that it is a distant galaxy. The object exhibits redder colors, indicating an older stellar population and a relatively low rate of star formation.
