The galaxy presents a primarily smooth, elliptical morphology. Its light profile appears relatively uniform, lacking prominent spiral arms or a distinct bar structure. The core region exhibits a concentrated luminosity, suggesting a high stellar density, possibly indicative of a supermassive black hole. The overall color index suggests a population of older, redder stars, implying a low star formation rate within the galaxy. There is slight visual evidence of minor disturbances of a tidal nature, however it does not appear to be undergoing a major merger event.
