The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy at a considerable distance, as indicated by its redshift. It exhibits a generally round morphology with a high degree of central concentration. There is no obvious spiral structure or significant disk component visible in this imaging, suggesting a lack of recent major mergers. Faint color variations indicate possibly an aging stellar population. No significant signs of ongoing major star formation can be discerned. It appears to be a typical, quiescent elliptical galaxy.
