The galaxy presents as an elliptical or lenticular morphology, exhibiting a largely smooth and centralized light distribution. Its overall shape is elongated, with a noticeable major axis. The light appears most concentrated toward the galactic center, which shows a bright and concentrated bulge. There is a subtle colour gradient visible, with the central regions appearing yellower and the outer regions becoming slightly bluer, potentially indicating a difference in stellar populations, such as the presence of younger stars at a low star formation rate in the outer disk. There are no obvious signs of tidal tails or major disturbances, suggesting it is not actively undergoing a major merger event. The galaxy appears relatively isolated, with no immediate companion galaxies noticeably interacting. The object appears to be at a considerable distance, evidenced by its small apparent size and redshift.
