The galaxy presents as a system undergoing a significant merger event. Evident is a disturbed morphology, with an elongated structure exhibiting asymmetrical light distribution. There appears to be a primary concentration of light, possibly a galactic nucleus, displaying a redder hue, indicative of older stellar populations and/or dust obscuration. Emanating from this central region are fainter extensions, one displaying bluer tones, suggesting regions of more active star formation. These features suggest ongoing tidal interactions between multiple galaxies. The system displays moderate to high luminosity and a size consistent with a galaxy of considerable mass. The overall color profile indicates a mixed population of stars with both young and old stellar populations contributing to the observed light.
