This galaxy appears to be in the process of merging, exhibiting a dual-core structure. Both cores present a smooth, elliptical morphology. The larger core is slightly more diffuse and exhibits a yellowish hue, potentially indicating an older stellar population. The smaller core is more compact and has a reddish color, possibly indicating dust or a population of younger stars. There is a faint tidal tail or bridge of material extending between the two cores, suggesting gravitational interaction. Overall, the system shows signs of significant disturbance.
