The galaxy displays an irregular morphology, likely indicative of an ongoing or recent merger event. Two distinct nuclei are observed, with a moderate amount of light concentrated in the central region of each.

Diffuse light extends outwards from the central regions, forming an irregular, asymmetric shape. Filamentary structures are discernible, suggesting tidal tails or disrupted spiral arms as a result of gravitational interactions. These features display a lower surface brightness compared to the central regions.

The color gradients within the galaxy are subtle. There is a slight bluer hue along the edges of the tidal features, potentially indicating regions of more active star formation. The central regions appear slightly redder, consistent with an older stellar population or increased dust obscuration.

Overall, the galaxy exhibits significant morphological disturbances characteristic of a system undergoing a merger or strong tidal interaction.
