The galaxy presents an overall elliptical morphology, elongated with an approximate axis ratio of 2:1. Its light profile appears relatively smooth and concentrated towards the center. There is a slight blue tint to the galaxy suggesting some level of ongoing star formation, but the dominant color is more typical of older stellar populations. There are some minor disturbances, with a slight hint of asymmetry which could be the result of a weak interaction with another galaxy. There is no clear indication of strong tidal features, a disk structure, or a prominent bulge.
