The galaxy appears to be a relatively smooth, elliptical or lenticular system at a considerable redshift. It exhibits a concentrated central bulge that is bright and yellowish-white in color, suggesting an older stellar population. The overall morphology presents a roughly rounded profile, with little indication of spiral arms or significant disk-like structure. No signs of ongoing major merger activity or tidal disturbances are readily apparent, but the possibility of minor interaction cannot be ruled out. The colors suggest moderate levels of star formation are occurring within the galaxy. Overall, the galaxy appears to be a massive system, relatively quiescent in terms of star formation.
