The galaxy presents as a dual-core system or interacting galaxy pair. One component exhibits a bright, blue-shifted region indicative of active star formation. This area appears somewhat clumpy or irregular in shape. The second component displays a smoother, more diffuse appearance with a redder color profile. This suggests an older stellar population and less active star formation. There appears to be a slight distortion of the overall shape of the system, possibly indicating a minor gravitational disturbance or early stage merger.
