The observed galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction. The central region displays a yellowish-orange hue, indicative of an older stellar population, potentially a bulge component. Faint, diffuse features extend from the central region, which may be indicative of tidal tails or distorted spiral arms. The overall structure deviates significantly from a standard elliptical or spiral morphology. The luminosity appears moderate, though the precise distance would be required to determine the absolute magnitude. Star formation seems present, but not dominant based on the colors. There is a secondary, smaller concentration of light and color below the main body. The image shows evidence of possible recent interaction. 
