This galaxy appears to be undergoing a significant interaction, possibly a merger. There are two distinct luminous cores, indicating the presence of two separate galactic nuclei. The light from the nuclei is yellowish and seems to be dominated by older stellar populations.  A more diffuse, bluish component surrounds each core, hinting at regions of ongoing or recent star formation, although the overall star formation rate seems relatively low. The general morphology is somewhat irregular, and the overall shape is not well-defined. There is a clear departure from a typical elliptical or spiral structure, suggesting a system in a state of dynamic evolution.
