The galaxy exhibits a distinct disk-like structure with a bright, concentrated central bulge. The primary color of the disk appears to be a shade of cyan, possibly indicating active star formation or a significant population of hot, young stars. The central bulge is slightly brighter than the disk, and is not well-defined. There are several artifacts in this image, but the galaxy does not show signs of tidal tails or major distortions, suggesting it is not currently undergoing a major merger event.
