The galaxy presents a complex morphology, possibly indicative of an ongoing interaction or merger. One component appears to be a relatively smooth, elliptical-like object with a yellowish-white hue, suggesting an older stellar population and a lack of significant ongoing star formation. The second component exhibits a bluer color, implying the presence of younger, hotter stars and active star-forming regions. This component appears more elongated, with a hint of disrupted structure. The red shift of this galaxy suggests that it is a distant galaxy.