The galaxy appears to be an interacting system, possibly in the early stages of a merger. There are two distinct nuclei, with one being more compact and centrally located within a diffuse, smooth envelope. The second nucleus appears smaller and less defined, located to the lower right of the primary nucleus. The color gradient suggests potential differences in stellar populations within the two components. The main body of the galaxy exhibits a somewhat disturbed morphology. There is evidence of tidal features or faint extensions emanating from the central region, which could be indicative of gravitational interactions. Overall, the galaxy displays a complex and dynamic structure likely driven by the ongoing merging process. Further investigation, potentially with spectroscopic data, could reveal more details about the stellar populations, gas content, and star formation activity within each component, shedding light on the merger's evolutionary stage.
