The galaxy appears as a concentrated, singular body with a smooth light distribution. There is a slight ellipticity to its form, though it appears relatively rounded. The color is predominantly yellow-orange, suggesting an older stellar population. There is no visible evidence of spiral arm structure or significant dust lanes, but its structure appears rather uniform and undisturbed. Based on these characteristics, it could be classified as an elliptical galaxy. Furthermore, no obvious tidal features or signs of ongoing mergers are observed.
