The galaxy exhibits a morphology consistent with a merging system. The primary component presents a relatively smooth profile and is elliptical in shape. It displays a red hue, potentially indicating an older stellar population and suppressed star formation activity. A second, less defined component is visible, displaying a yellower color, potentially suggesting a different stellar population or dust content. There is a slight possibility of a disk structure, though difficult to confirm with the resolution. This system is interacting, as there are minor visual disturbances. The observed colours suggest a more complex, active history, with potential for a wide range of stellar ages present within each component.
