The galaxy appears to be a complex system, potentially interacting with another galaxy. There are two distinct luminous regions, one appearing slightly more extended and diffuse than the other. Both regions exhibit a general blue-white color indicative of relatively young stellar populations or active star formation. The central regions show hints of a disk-like structure. There is evidence of a diffuse, surrounding halo of light extending beyond the primary luminous regions. This suggests a potentially older stellar population in the outskirts of the galaxy. Overall, the system's morphology is somewhat disturbed, hinting at an ongoing or recent interaction. There is some asymmetry to the brightness distribution, particularly in the fainter region. This further supports the hypothesis of an ongoing merger or tidal interaction.
