The galaxy appears as a single, relatively smooth, and concentrated light source, with a hue tending towards yellow-red, suggesting an older stellar population. Its morphology is generally elliptical. There is minimal observable structure, such as spiral arms or prominent dust lanes, implying that the galaxy lacks significant on-going star formation. The absence of discernible tidal features suggests it is relatively undisturbed gravitationally and not currently undergoing a major merger event. Its round appearance indicates it is likely viewed close to face-on.
