The galaxy appears relatively small and faint. It exhibits a disk-like morphology, with hints of spiral arm structure, though somewhat disrupted. The overall color is slightly red-shifted with some blue areas scattered sparsely, indicating the presence of both older stellar populations and regions of recent star formation. The galaxy may be undergoing a minor interaction or disturbance given the asymmetry present in the spiral arm structure. The central bulge is not particularly prominent, suggesting it may be a late-type spiral. The galaxy shows evidence of a merger event or strong tidal interaction. This has significantly affected the morphological structure of the galaxy.
