The observed galaxy appears to be a merging system. There's a primary, relatively smooth, elliptical-like component, exhibiting a diffuse, albeit somewhat disturbed morphology. The color suggests a population of older stars, possibly with some recent star formation as indicated by the slight bluer tinge. A secondary, smaller component is visible in close proximity, indicating an ongoing or recent merger event. The primary component appears somewhat elongated, lacking a clear disk structure. There is likely a supermassive black hole contained in this galaxy. The rate of star formation appears to be low, implying that the majority of star formation occurred in the past. The system presents a moderate luminosity, hinting at a smaller galactic structure.
