This galaxy presents as a somewhat amorphous, distorted structure, potentially indicative of an ongoing interaction or past merger event. The central region exhibits a degree of smoothness. Extending outwards, there are clear signs of tidal disturbances, manifesting as faint, diffuse structures and asymmetries in the overall shape. A dominant blue hue throughout the main body suggests active star formation and a younger stellar population. The morphology leans towards a disk-like appearance when looking at how the galaxy lays on the image plane, although this shape is significantly disrupted. There may be a companion galaxy, which could be contributing to the observed disturbances. Overall, this galaxy displays characteristics consistent with a system undergoing a dynamically active phase, likely driven by gravitational interactions.
