The galaxy presents a primarily smooth, elliptical morphology. The core exhibits a high degree of sphericity and is intensely luminous, appearing a yellow-orange hue. The galaxy displays a significant red shift, indicative of a substantial distance. There is a slight asymmetry apparent, with some subtle disturbances in the outer regions, indicating possible minor interactions or past mergers. The galaxy's overall color suggests an older stellar population and a suppression of current star formation activity.
