This galaxy appears to be undergoing a significant interaction or merger. The overall morphology is disturbed, showing a complex structure with irregular features and tidal tails are potentially present.

There is a bright central region with a yellowish hue, suggesting an older stellar population and/or dust obscuration in the core. The outer regions show a bluer color, indicating the presence of younger, hotter stars potentially formed by the interaction or merger event. There is a fainter secondary object to the side that may be either a separate galaxy interacting with the larger one, or a tidal dwarf galaxy formed by the merger. The system has a moderate size and luminosity. The irregular shape and color gradients suggest ongoing star formation activity triggered by the interaction.
