The galaxy presents as a somewhat diffuse object, exhibiting characteristics that suggest it is undergoing a significant interaction, potentially a merger. The morphology appears disturbed, lacking a clear, well-defined structure. There is an extended, elongated feature with a faint, diffuse halo, possibly indicative of tidal debris or a disrupted disk. A secondary, brighter, and more compact component is observed near the extended feature, connected with the larger galaxy by a faint stream of light. This could represent the core of the secondary galaxy in the merger, or a dense region of star formation triggered by the interaction. The overall color is a muted blue, potentially indicating the presence of younger stellar populations.
