The galaxy presents as a system of two distinct components. The larger component exhibits a smooth, elliptical morphology, appearing elongated in shape. Its color profile suggests a population of older stars, with a yellowish-red hue dominating. There is no visible spiral structure or dust lanes. The smaller component presents a smoother and more compact morphology, but with a more bluish color, hinting at a younger stellar population. It's possible the overall system is undergoing some gravitational interaction given the disturbed morphology. The galaxy is estimated to be relatively massive with moderate levels of star formation.
