The galaxy exhibits a morphology suggesting an ongoing or recent merger event. The overall structure is disturbed, lacking a clear, defined shape. There is evidence of multiple interacting components, potentially multiple galactic nuclei or dense star-forming regions. The light distribution suggests a mix of stellar populations, with some areas appearing redder, potentially indicating older stellar populations or dust obscuration, and other regions showing a bluer hue, which may be indicative of younger, hotter stars forming. The galaxy is relatively compact in size, with a moderate luminosity. Given the apparent disturbances, it is reasonable to infer that the galaxy is undergoing elevated star formation activity, although this is not directly observable from the image alone.
