This galaxy appears to be an interacting system, potentially in the early stages of a merger. It is characterized by a disturbed morphology, lacking a clear, well-defined structure. There are two distinct, luminous components visible. One component is elongated, possibly a disk that is not viewed edge on, with a smooth appearance. The other component is more compact and spherical, potentially the nucleus of another galaxy. There is faint tidal debris or distortions are observed suggesting gravitational interaction. There is a hint of bluer regions, perhaps indicating ongoing star formation. The system appears to be relatively small, with an estimated effective radius of a few kiloparsecs. Overall, the galaxy exhibits characteristics suggesting a complex evolutionary history involving galaxy interactions or mergers, that are in the process of disrupting its original structure and potentially triggering star formation activity.
