The galaxy appears as a compact, relatively small structure with a somewhat irregular shape. There are no discernible spiral arms or a defined galactic disk. The light is dominated by a central, bright region, possibly indicating an active galactic nucleus or a high concentration of stars. The overall color of the galaxy is bluish, suggesting the presence of younger, hotter stars. This is contrasted by a less-defined area of pinkish color, indicating the presence of HII regions where star formation may be happening. 

The morphological classification seems to lean towards a galaxy with interacting features, or at the very least, a system exhibiting structural disturbances, which could mean it is undergoing a merger event.
