The galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a generally round morphology. There is a subtle blue color gradient present, particularly towards the outer edges of the galaxy, suggesting the presence of some younger stellar populations, even if they are not dominant. The galaxy displays no obvious signs of spiral arms or significant disk features. It seems to be fairly isolated, lacking any major disturbances or clear indications of an ongoing merger event. The galaxy shows a concentrated central region with a gradual decrease in surface brightness moving outwards. Overall, the galaxy appears to be a fairly massive and luminous galaxy at a considerable distance. Its light is redshifted due to the expansion of the universe, placing it at a significant cosmological distance. The estimated size is on the order of several kiloparsecs across. Despite its relatively smooth appearance, subtle color variations imply some level of ongoing or recent star formation activity, but it's likely at a very low rate.
