The galaxy appears as a relatively smooth, rounded structure. There is a concentrated central bulge that exhibits a bright, mostly white-yellowish hue. The outer regions show a gradual decrease in luminosity, transitioning into a diffuse, somewhat bluish envelope. There are no prominent spiral arms or distinct features visible, suggesting a lack of ordered structure, or that any such structure is obscured by distance or dust. The overall form is elliptical, bordering on lenticular, lacking sharp boundaries. There is no apparent active galactic nucleus, or tidal disruption, which suggests it has been undisturbed for a long time.
