This galaxy appears to be undergoing a significant interaction or merger. The morphology suggests two distinct nuclei or regions of high stellar density, possibly representing the cores of two progenitor galaxies. There are indications of tidal features, such as faint extensions or distortions, which are characteristic of gravitational interactions between galaxies. The object exhibits a diverse range of colors, with some regions appearing bluer, indicating younger stellar populations and active star formation, while others are redder, suggesting older stellar populations. Overall, this is an intermediate-mass, actively star-forming system in a state of dynamic evolution.
