The galaxy exhibits a disturbed morphology, suggesting a possible ongoing or recent merger event. Two distinct luminous cores are visible, potentially representing the nuclei of the merging galaxies. The overall shape is somewhat rounded, but significantly distorted compared to a typical elliptical galaxy. The color profile indicates a redder population indicative of older stars, but shows some bluer features concentrated in the core, suggesting ongoing or recent star formation in localized regions. The galaxy appears to be relatively large, potentially a massive system. Faint tidal features are not apparent. A merging classification seems appropriate.
