The galaxy presents as a system with multiple interacting components. A central, bright, and roughly spherical component dominates the apparent luminosity. This core exhibits a distinct color gradient, transitioning from a bluish-white halo toward a more concentrated purple at its center, suggesting variations in stellar populations or dust extinction.

Extending outwards from this central region, there's a suggestion of a fainter, more diffuse structure. A less luminous, yellowish structure is visible, possibly indicative of a disk-like or tidal feature. The overall shape is irregular, showing hints of possible gravitational interactions. There is evidence of disturbance in the morphology.
