This galaxy appears to be undergoing a significant merger event. The primary body of the galaxy presents a somewhat smooth profile but exhibits a disturbed morphology indicative of gravitational interaction. A second, smaller, and brighter core is visible, suggesting the presence of another galaxy actively merging with the larger one. The overall color of the system tends towards yellower and redder hues, which may be indicative of a galaxy with a significant population of older stars. The distribution of light suggests some tidal features and asymmetries, with the distinct possibility of tails or bridges extending outward from the core regions, though these are not sharply defined. Overall, the system displays characteristics of a major merger in progress, disrupting the original galactic structure.
