The galaxy presents a complex morphology, appearing as a potential merger event. Two distinct components are visible. One component exhibits a smoother, more rounded profile, with a yellowish-orange hue suggesting an older stellar population and/or significant dust obscuration. The second component displays a brighter, slightly elongated structure with a blue-green tint, indicative of ongoing or recent star formation. There are indications of tidal interactions, with some faint extensions or disturbances emanating from both components. The galaxy is overall quite compact. The colors of the components are quite distinct, suggesting possible variations in metallicity.
