The galaxy presents a complex morphology, appearing as a dual-core structure, potentially indicative of an ongoing or recent merger event. Each core exhibits a diffuse, elliptical shape, with a noticeable concentration of light towards the center, suggesting the presence of galactic nuclei. The color distribution within the galaxy shows a general redder hue, concentrated near the center, hinting at a population of older stars. The outer regions exhibit fainter, bluer tinges, which might indicate more recent star formation, particularly within the tidal features. The overall structure appears somewhat disturbed, with faint extensions or tidal tails visible, further supporting the merger hypothesis. The galaxy's overall smoothness suggests that it is approaching the later stages of this major merger process, and it shows signs of an elliptical galaxy morphology with an oblate shape.
