The galaxy appears to be a luminous, early-type system, likely an elliptical or lenticular galaxy. It exhibits a smooth, centrally concentrated light distribution with a high degree of circular symmetry. There is no discernible spiral arm structure or prominent dust lanes. Faint, diffuse light extends outward from the core, suggesting a relatively large effective radius. There is potentially some ongoing merger activity occurring within the galaxy's halo, or small tidal disturbances. Overall, the galaxy shows characteristics of a relatively evolved, passively evolving system with a high stellar mass and little to no current star formation.
