The galaxy appears to be a relatively smooth, elliptical system. The light profile suggests a centrally concentrated bulge component, gradually fading outwards. There is a slight ellipticity but it appears mostly rounded. Faint blue hues are detected in the outer regions, perhaps indicating areas of modest recent star formation, but the bulk of the galaxy appears composed of older stellar populations giving it a yellowish-white core. No distinct spiral arms or bar features are visible. There are no obvious signs of a major ongoing merger, or significant tidal disturbances in the immediate vicinity.
