This galaxy exhibits a slightly elongated morphology. The central region displays a concentrated brightness, potentially indicative of an older stellar population, which fades into a more diffuse halo or disk-like structure extending outwards. There is a faint blueish arm present, suggesting recent star formation. I can also see some indications of minor tidal disturbances or interactions affecting the galaxy's overall shape; there may be a potential companion galaxy as well. The galaxy is a relatively luminous object and has a red shift greater than zero, and has a estimated diameter of a good size. It is moderately smooth with some disk-like structures with an artifact fraction suggesting possible image artifacts or processing challenges. Some of the image suggests it might be in the process of merging.