This galaxy exhibits a generally elliptical morphology, appearing mostly smooth with a high degree of central concentration. It is quite luminous, showing a bright yellow-white core indicative of an older stellar population. Fainter light extends outwards forming a larger halo. There appears to be some degree of merging, as there is some disturbance on the top of the galaxy. Overall, the galaxy has no clearly visible spiral arms or a distinct disk structure and is relatively round. Its red shift places it at a considerable distance. This is most likely a relatively massive galaxy with a low star formation rate.
