The galaxy exhibits a complex morphology, appearing as a potentially interacting system. Two primary luminous components are discernible, exhibiting an orange-yellow hue suggestive of an older stellar population with relatively low ongoing star formation. One component displays a more compact and rounded shape, while the other appears slightly elongated or distorted. A faint, diffuse envelope of light surrounds these components, potentially indicative of tidal debris resulting from gravitational interactions. The overall structure hints at an ongoing or recent merger event. The system presents a moderate redshift.
