The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a noticeable decrease in surface brightness radiating outwards from the core. The color is predominantly yellow, suggesting an older stellar population. The galaxy displays a moderate degree of roundness. There are no strong indications of spiral arm structures or prominent dust lanes. No clear sign of an ongoing major merger event is apparent, though minor disturbances may be present given the slightly irregular shape. The redshift indicates that this galaxy is at a significant cosmological distance.
