The galaxy appears to be undergoing a significant interaction, potentially a merger. Two distinct, yet closely associated, components are readily visible. One component presents a bluish hue, indicative of recent star formation. The other component exhibits a yellower coloration, suggesting an older stellar population. The bluish component seems elongated, possibly a tidal tail resulting from the gravitational interaction. There are no well-defined spiral arms, although hints of structural distortion are evident, particularly around the periphery. Overall, this system presents as a disturbed and complex morphology, indicative of an ongoing or recent gravitational interaction.
