The observed galaxy exhibits an apparent morphology indicating a system undergoing a merger. Two distinct luminous components are discernible. The primary component is roughly circular in shape with a smooth appearance and a yellowish hue, suggesting an older stellar population and diminished star formation activity. The secondary component, located in close proximity to the primary component, appears less defined, with a more irregular shape and a slight elongation. The overall color of the secondary component is also slightly more red-shifted, which may indicate a more evolved stellar population compared to the primary component. There's no presence of prominent spiral arms or a well-defined disk structure in either of the components. The system overall appears to be compact and relatively isolated. A significant fraction of the Galaxy Zoo classifications suggests ongoing or recent merger activity, further supporting this interpretation of the system's current state.
