The galaxy exhibits a morphology characterized primarily by apparent disturbances, suggestive of potential gravitational interactions. A significant portion of the galaxy's light is distributed irregularly, indicating an evolved system undergoing active processes. Evidence supports the presence of merging or tidal interactions. The galaxy appears elongated, with a noticeable asymmetry in its structure. Patches of brighter, more intense luminosity are interspersed with fainter, diffuse regions. The overall color profile shows a complex interplay of wavelengths, hinting at varying stellar populations and dust content across the galactic body. A merger may be occurring in the system.
