The galaxy presents an overall elliptical morphology, appearing relatively smooth in structure. It exhibits a slight elongation, though it tends towards a round shape. There is evidence of a brighter, more concentrated central region, likely the galactic nucleus, which appears to have a yellow-white hue. This core is surrounded by a fainter, more diffuse halo. The galaxy shows a red-shift indicating it is at a significant cosmological distance. There is a potential for minor morphological disturbances, but no definitive signs of a major merger event are observed. It appears to be a relatively low-mass system with a correspondingly low star-formation rate.
