The object appears to be a system of gravitationally interacting galaxies, possibly in the early stages of a merger. The largest component is a centrally concentrated, elliptical galaxy with a smooth, relatively featureless morphology. Its color is slightly redder, suggesting an older stellar population with less active star formation.

There are two less massive components, one appearing bluish-white, and the other a faint streak of light. They show a disk-like morphology and are bluer in color, indicative of younger, hotter stars and ongoing star formation. These galaxies are closer together than the elliptical, hinting at a later merger stage in this subsystem.

The system shows signs of gravitational disturbance; no distinct tidal tails are apparent. The absence of prominent tidal features might indicate an early stage of interaction or that the tidal debris is too faint to be detected at this resolution.