This galaxy presents as a relatively smooth and elongated elliptical galaxy. It appears to be dominated by an older stellar population, with a central concentration of light indicating a bulge. The light is rather uniform with the color suggesting little current star formation. The galaxy shows no prominent dust lanes, spiral arms, or other features indicative of recent mergers or significant gas content. The light distribution gradually fades outwards, indicating a diffuse halo component. There appears to be no significant tidal disturbance or interactions with neighboring galaxies. The overall color is consistent with what is expected of a galaxy at its estimated redshift.
