The galaxy presents an irregular morphology, with visible signs of disturbance and potential merging activity. The object appears to be undergoing a significant interaction, as evidenced by the non-symmetric light distribution and presence of tidal features. There is an irregular shape with extended faint emission. These features suggests ongoing gravitational interaction with another galaxy or recent merger event. There may be a disk-like structure. The galaxy color suggests a mix of stellar populations, with both older, redder stars and younger, bluer stars present, concentrated in different regions. Further spectroscopic analysis would be beneficial to understand the kinematic and metallicity of these regions.
