The galaxy exhibits a disturbed morphology, indicative of an ongoing or recent merger event. Two distinct luminous components are visible. The larger component is elongated, with a yellowish hue, suggesting an older stellar population. The smaller component has a similar color profile, although it is less well-defined. The shape of the system departs significantly from a regular elliptical or spiral structure, appearing highly asymmetric. There is a faint halo of diffuse light surrounding the primary components, possibly representing tidal debris resulting from the interaction. Overall, the system is dominated by older stars.
