The galaxy presents a complex morphology, potentially exhibiting characteristics of both a disk galaxy and a system undergoing a merger or interaction. The central region displays a relatively smooth, concentrated appearance suggesting an older stellar population. Surrounding this core, the galaxy's structure becomes more complex, with evidence of a faint disk-like structure and possible tidal features. The bluer colors of the outer regions suggest the presence of younger, hotter stars, possibly indicating ongoing or recent star formation activity in these areas. Irregularities in the galaxy's shape, and the presence of diffuse light extending beyond the main body suggest a dynamic history, possibly involving gravitational interactions with another galaxy. There is evidence of a possible merging event or significant disturbance of the galactic structure. The galaxy exhibits a moderate level of star formation.
