The galaxy appears to be undergoing a merger, likely between two distinct galaxies. A larger, more diffuse component exhibits a yellowish hue, suggesting an older stellar population. This is in close proximity to what appears to be a smaller, more compact, and bluer component, indicating ongoing or recent star formation.

The morphology is clearly disturbed, lacking a well-defined structure. There is evidence of tidal interactions, with a faint extension or bridge of material connecting the two components. The overall shape is elongated and irregular, and the merging process may result in the formation of an elliptical galaxy.
