The galaxy presents as a relatively smooth, elliptical morphology. There appears to be minimal or no evidence of spiral arm structure. The light distribution is concentrated towards the center, with a bright, compact core indicative of a high stellar density. The galaxy exhibits a gradual decrease in luminosity from the core outwards, forming a diffuse halo. Subtle color gradients are observed, with the central region displaying a slightly yellowish or reddish hue, potentially indicating an older stellar population. The outer regions appear somewhat bluer, which might be caused by a small amount of younger stars or ongoing, low-level star formation. There are no obvious signs of active galactic nuclei or strong starburst activity in this image. No significant distortions or tidal features suggest recent major merger events. The overall appearance suggests a galaxy that is relatively evolved and quiescent.
