The object appears to be a galaxy at a considerable distance, evidenced by its small angular size and redshift. It exhibits a generally smooth morphology, with a centrally concentrated luminosity profile. The galaxy's light is dominated by a yellow-orange hue, with hints of green at the edge, indicative of an older stellar population and a lower rate of on-going star formation. There is no clear evidence of spiral arms or a distinct disk structure, and the overall shape is quite round, lending support to an elliptical classification. Subtle variations in color and surface brightness suggest minor disturbances, possibly past or ongoing interactions.
