The galaxy presents a generally elliptical morphology. Its light is centrally concentrated, appearing brightest towards the core, with a gradual decrease in luminosity outwards. The overall color is yellowish-orange, suggesting a stellar population dominated by older, redder stars. There is little indication of prominent spiral arm structure or significant dust lanes, lending further credence to a relatively smooth, potentially early-type classification. No apparent signs of active galactic nuclei activity or recent major merger events are observable from this image. There are subtle hints of a slightly elongated shape, though the deviation from perfect circularity appears minimal.
