This galaxy appears to be undergoing a significant interaction or merger. The morphology is highly disturbed and irregular, lacking a clear central bulge or defined spiral arms. There are multiple bright knots or clumps of stellar material distributed throughout the galaxy, suggesting intense star formation activity. These clumps vary in color, with some exhibiting a redder hue, indicative of older stellar populations or dust obscuration, while others appear bluer, suggesting younger, hotter stars. The overall light distribution is relatively diffuse, with no distinct boundaries. There appears to be tidal features or extended plumes of material emanating from the main body of the galaxy, further supporting the hypothesis of an ongoing merger. The galaxy exhibits a broad spectrum of colors, with a general trend toward redder wavelengths dominating.
