The galaxy presents as a system with a dominant, seemingly smooth central component. This core exhibits a yellowish-white hue, suggesting an older stellar population. The overall light distribution appears relatively concentrated. A faint disk-like structure can be observed, though it's not sharply defined and constitutes a small fraction of the total light. There are subtle asymmetries in the galaxy's morphology, with a faint, minor distortion. The color variation across the galaxy is subtle. It has a round shape. The galaxy displays a relatively low level of on-going star formation. There is no presence of a prominent tidal tail or other significant signs of a recent major merger event.
