The galaxy presents as a single, relatively smooth, and concentrated body of light. The overall shape is elliptical, with a major axis discernable, though it appears only slightly elongated. The light profile suggests a higher concentration of stars towards the galactic center, which emits a yellowish-white glow. The outer regions appear less luminous and exhibit a more reddish hue. There is no strong evidence of spiral arms or a prominent disk structure. There is also no obvious sign of intense star formation regions or dust lanes. The galaxy exhibits no clear signs of major tidal disturbances or active galactic nucleus activity based on the image alone. Overall, the visual appearance of the galaxy is consistent with an elliptical morphology, likely a mature system with an older stellar population.
