The galaxy appears as a centrally concentrated, elliptical-like object. It exhibits a smooth, diffuse light distribution with a subtle color gradient, transitioning from a yellowish-white core to a slightly bluer outer region. There is no obvious spiral arm structure or dust lane. The central region is brighter and more condensed, likely indicating a higher concentration of older stars. The outer regions appear more diffuse and less concentrated, suggesting a gradual decrease in stellar density with increasing radius. The overall morphology suggests a system that is either a relatively undisturbed elliptical galaxy or possibly a late-stage spiral galaxy that has undergone significant morphological transformation. There's a hint of disturbance in the morphology.
