The galaxy presents as a centrally concentrated object with a generally elliptical morphology. Its core region exhibits a bright, yellowish-orange hue that fades into a dimmer, greenish corona. The light distribution appears largely smooth, with a high degree of radial symmetry. There is no strong evidence of spiral arms, a prominent disk, or any significant tidal features in the surrounding area that may suggest a recent major merger event, though there is a slight asymmetry in the extension of the green corona. The overall color profile suggests a relatively evolved stellar population with potentially suppressed star formation. The observed characteristics are generally consistent with an early-type galaxy, likely a lenticular or elliptical galaxy at moderate redshift.
