The galaxy appears as a centrally concentrated, relatively smooth object. Its overall shape is elliptical, close to circular. The light distribution suggests a dominant bulge component with a gradual fading towards the outer regions. There is a color gradient, with the core appearing whiter and the outer regions appearing more reddish. No distinct spiral arms or significant dust lanes are visible. The galaxy doesn't show any signs of major disturbances or merging activity. Faint indications of some irregularities could suggest past or minor interaction events.
