The galaxy appears to be an interacting system comprised of two distinct galaxies. The primary galaxy exhibits a disturbed morphology, showing signs of gravitational interaction with its companion. The larger galaxy has a mostly smooth appearance, though there are visible deviations from perfect elliptical symmetry.

A smaller companion galaxy is visibly interacting with the larger one. The smaller galaxy has a bluer color, which suggests it has a higher amount of on going star formation. There appears to be faint tidal tails and debris connecting the two galaxies, indicating an ongoing merger event.

The overall color of the system suggests a mixed stellar population, with both older, redder stars and younger, bluer stars present. The system exhibits a relatively compact structure. There is no strong evidence of a prominent disk component.