The galaxy presents as a relatively smooth, centrally concentrated object. The morphology is most likely that of an elliptical galaxy, with a discernible but faint extended halo. The core of the galaxy shows high luminosity, with light output diminishing gradually towards the outer regions. The shape appears elongated, possibly cigar shaped, indicating it is not perfectly spherical. There are no obvious signs of spiral arms or significant dust lanes. There are no indications of tidal tails or strong gravitational disturbances, suggesting it is not undergoing a major merger. The overall color indices suggest the presence of both older stellar populations and modest star formation activity. Overall, the galaxy exhibits characteristics consistent with a large elliptical galaxy, exhibiting a small amount of star formation.
