The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits a largely elliptical morphology, with a high degree of roundness. No distinct spiral arms or bar structures are apparent. The core region is dominated by a bright, yellowish-white light, which is likely from an older stellar population. There is a subtle decrease in the surface brightness from the center moving outwards. Additionally, there are hints of a slight disk feature to the galaxy. The galaxy is isolated and shows no evidence of recent or ongoing major mergers or tidal disturbances, although some minor disturbances may be present. The redshift indicates the galaxy is at a substantial cosmological distance.
