The galaxy appears to be in the late stages of a merger, possibly with another galaxy of similar size. It has a relatively smooth overall appearance, but exhibits significant tidal distortions. A diffuse, extended halo surrounds the primary luminous region, indicating gravitational interactions are disrupting the galaxy's original form. There is an apparent concentration of light in two distinct central regions, which could be the remnant cores of the merging galaxies. The color is generally redder than typical spiral galaxies, suggesting an older stellar population, indicative of a diminished star formation rate within the system.
