The galaxy appears as a relatively smooth, elliptical structure. The light profile suggests a concentrated central bulge that gradually fades outwards. The color gradient indicates a redder core region, transitioning to slightly bluer hues in the outer regions. There is a lack of distinct spiral arm structures or prominent dust lanes, which is consistent with an elliptical morphology. There is a small indication of tidal disruption, but this is likely a normal looking elliptical galaxy. Given the redshift, we are observing this galaxy at a considerable distance, implying a significant intrinsic luminosity.
