The object appears to be a galaxy at a considerable distance, evidenced by its small angular size and redshift of 0.266159. It presents an elliptical morphology, appearing mostly smooth with a high degree of central concentration, though some slight disk-like structure can be observed. The galaxy's light profile suggests a largely homogenous stellar population throughout the galaxy. The color index indicates a possible lack of ongoing, intense star formation, showing redder colors. There may be signs of a minor galactic disturbance. The object could be considered a massive, relatively evolved galaxy.
