The galaxy exhibits an irregular morphology, with an apparent disturbed structure. There is evidence of a possible ongoing merger or interaction. The system presents with a dual or multi-component core, suggesting the potential presence of multiple galactic nuclei. The overall color appears to be relatively red, which could indicate an older stellar population or significant dust extinction. There may be faint tidal features or extended emission surrounding the main body of the galaxy; these are not distinct, but can be observed near the brightest components. The overall structure does not clearly resemble a typical spiral or elliptical galaxy, given its disturbed and asymmetric appearance.
