This galaxy exhibits characteristics suggesting an ongoing or recent merger event. The primary body of the galaxy appears diffuse and somewhat amorphous, lacking a distinct spiral or elliptical structure. Two prominent, centrally concentrated regions of high luminosity are observed, implying the presence of two distinct galactic nuclei in close proximity. These bright regions exhibit a yellowish hue. The overall color gradient across the galaxy tends towards redder wavelengths. No visible dust lanes are present. The surrounding halo demonstrates signs of tidal disruption, indicating gravitational interaction and material stripping from the primary galaxy.
