This galaxy, as observed, presents a fairly smooth, elliptical morphology, exhibiting a centrally concentrated light profile. The color index suggests a population of older stars, lending to the galaxy's yellow-red hue. There are no prominent spiral arms or distinct dust lanes visible. There is no apparent active galactic nucleus and no obvious signs of a recent major merger event; however, a slight asymmetry or minor disturbance in the overall structure cannot be fully ruled out.
