The galaxy appears to be a relatively smooth, elliptical galaxy. Its overall form is generally rounded, with a concentrated central bulge that emits significant light. The color gradient suggests a population of older stars, possibly lacking in substantial ongoing star formation within the galaxy's main body. Faint outer regions are visible, which indicates a spread-out stellar distribution, but there is no obvious spiral structure or strong tidal features indicative of recent major mergers. A very small amount of disturbance is possible, but this is not a strong characteristic.
