The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy at a distance indicated by its redshift. It exhibits a yellowish-orange hue, suggesting a population dominated by older stars with lower rates of on-going star formation. There is a lack of discernible spiral arm structures or significant dust lanes. The overall morphology appears undisturbed, with no obvious signs of recent mergers or tidal interactions, although subtle minor disturbances cannot be ruled out at this resolution. The galaxy appears to be relatively round in shape.
