The galaxy appears to be undergoing a major merger. It exhibits a disturbed morphology, with a somewhat amorphous shape. There are two distinct, bright central concentrations of light that likely represent the cores of the progenitor galaxies. The overall color of the galaxy is relatively red, suggesting an older stellar population and potentially a significant amount of dust obscuration. There are indications of tidal tails or streams extending from the main body of the galaxy, further supporting the ongoing merger scenario. These features appear faint and diffuse. The galaxy does not show a clear disk structure; the light distribution appears more spheroidal and irregular, which could be due to the disruption caused by the interaction.
