The galaxy presents a largely smooth, elliptical morphology. The core is a bright, concentrated yellowish hue, suggestive of an older stellar population. There is an extended, less defined halo surrounding the core. The halo's color transitions to a more reddish tone at the edges. A slight asymmetry is observed, potentially indicating a minor gravitational disturbance or past interaction. The overall structure shows minimal signs of spiral arms or significant dust lanes. The smooth and featureless nature of the galaxy suggests a classification towards the elliptical end of the Hubble sequence.
