The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical with a high degree of roundness. There's a slight color gradient from the central region outward, shifting from a yellowish hue at the core to a more reddish tint in the outer regions. The galaxy does not appear to have any distinct spiral arm structures or significant dust lanes. There is no indication of a recent major merger event, although a minor disturbance or tidal feature cannot be ruled out completely due to the image resolution. The light profile suggests a relatively quiescent object with little ongoing star formation compared to the past, with older stellar populations dominating the overall light emitted, especially in the central part.
