The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. The core exhibits a bright, concentrated glow which suggests a higher density of stars or potentially an active galactic nucleus. Proceeding outward from the core, the intensity of light diminishes gradually without prominent spiral arm structures or distinct features. The outer regions blend into the background, indicating a diffuse stellar halo. The colouration appears predominantly blue-ish or turquoise, suggesting intermediate ages of stars with possibly ongoing, but subdued star formation. The general lack of significant tidal features or distortions indicate that the galaxy has experienced a relatively quiescent merging history.
