The galaxy presents a largely smooth, elliptical morphology. There is a concentrated central bulge, suggesting a substantial population of older stars. The overall color is yellowish-red, also indicating an older stellar population and diminished ongoing star formation. No distinct spiral arms or dust lanes are discernible in this image. There is no indication of any tidal tails or other features that would indicate a recent major merger event. There might be evidence of minor disturbances in the morphology. The galaxy appears fairly rounded with a slight ellipticity.
