The galaxy presents as an elongated, disk-like structure viewed at a significant angle. The central region exhibits a high degree of luminosity, appearing almost uniformly bright and nearly spherical. The outer regions show a gradual decrease in brightness, fading into the background sky. The color profile suggests a bias towards bluer wavelengths, especially within the central region, which is further indicative of possible ongoing or recent star formation activity. This might be suggestive of a spiral galaxy but the structure is distorted. There are visible disruptions to the galaxy’s symmetry suggesting there are possible merging features present.
