The object appears to be an elliptical galaxy at a considerable distance. It exhibits a smooth, largely featureless morphology, with a high degree of central concentration, exhibiting a yellowish hue, indicative of an older stellar population. The galaxy's overall shape appears roughly rounded, with no obvious signs of spiral arms or significant disk structure. The color suggests that star formation rates are relatively low. There appears to be minimal evidence of ongoing or recent major mergers or tidal disturbances impacting the galaxy’s structure.
