This galaxy appears to be in a late-stage merging process, with significant morphological disturbance evident. There is a primary, brighter component displaying a slightly elongated, though somewhat indistinct, morphology. Its color suggests a mix of stellar populations, possibly with ongoing or recent star formation.

There is a secondary, more compact object located very close to the main galaxy and connected by a small filament. The color of this secondary object appears yellower than the primary galaxy, implying an older stellar population.

Overall, the system exhibits moderate luminosity. The morphology suggests a complex interaction, and the presence of possible tidal features may be present, contributing to the distorted appearance. The relative proximity and disturbed features support the classification as a merging system.
