The galaxy presents an overall elliptical morphology, appearing relatively smooth and diffuse with a high degree of central concentration. It exhibits a subtle elongation, deviating slightly from a perfect circular shape. Some degree of dust absorption may be present, although it is not particularly pronounced. The light distribution suggests that it is a relatively massive galaxy with a high likelihood of being a quiescent or passively evolving system. Evidence indicates that the galaxy may be interacting with another galaxy, as the structure is somewhat disturbed. The object displays a faint, but non-negligible, blue component indicating some low-level ongoing star formation.
