The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge that graduates into a more diffuse halo. The overall color profile indicates a dominance of older stellar populations, suggested by the reddish-yellow hue of the galaxy. There's no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy's morphology suggests it is likely a mature system, possibly nearing or already at the red sequence. There is no obvious evidence of active galactic nuclei activity, strong tidal interactions, or recent merger events. It appears generally undisturbed.
