The galaxy presents as a diffuse object with a distinct, non-uniform morphology. It appears to have undergone a significant interaction or merger event. Evident are tidal features or disturbances indicating gravitational interactions, suggesting possible tidal tails or debris fields. These features exhibit a bluer hue, potentially indicative of younger stellar populations. The main body of the galaxy displays a central concentration of light, though it is not perfectly symmetric. There is a hint of a disk-like structure embedded within the broader, disturbed morphology. The overall color of the galaxy's central region appears slightly redder compared to the outer structures, possibly suggesting an older stellar population. The overall light distribution is asymmetric, with a brighter region and a more diffuse and fainter area, contributing to its disturbed appearance.
