The galaxy exhibits a morphology suggesting it may be in the process of merging or experiencing a tidal interaction. The main body of the galaxy appears relatively smooth, with a somewhat elongated shape. However, a distinct feature extends outwards from the primary structure, taking the form of a tidal tail or bridge. This secondary feature displays a bluer color compared to the main body, potentially indicative of a younger stellar population or ongoing star formation triggered by the interaction. There is some evidence of possible minor disturbance within the central region of the main galaxy body, but it otherwise appears to be largely smooth.
