The galaxy presents a somewhat diffuse, elliptical morphology. There is a subtle gradient in surface brightness, appearing brightest in the central region. It is difficult to ascertain if the structure is uniform, or if there are more complex features within, due to the resolution. A blueish tint can be observed implying the existence of younger, hotter stars. Its apparent small angular size and redshift suggest that this is a relatively distant galaxy. There is no obvious spiral arm structure or a prominent central bulge visible. Faint, possibly tidal, features may be present indicating an interaction, but this is uncertain. Overall, the galaxy appears to be a relatively normal elliptical galaxy. Further data, such as higher resolution imaging or spectroscopy, would be useful to determine its detailed composition and evolutionary state.
