The galaxy exhibits a relatively small angular size. It is likely a distant galaxy. The galaxy's morphology appears to be largely undisturbed, showing little evidence of major mergers or tidal interactions. A slight blue tint indicates the presence of young, hot stars. The core of the galaxy seems relatively compact. Evidence of disk structure is present, but not clearly resolved. There seems to be a smooth central bulge. Overall the galaxy is a spiral with slight disturbances.
