This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that gradually fades into a diffuse halo. The color gradient suggests an older stellar population, with the central region displaying a yellowish hue, possibly indicative of evolved stars. There is no distinct spiral arm structure visible, nor any indications of recent major merger events. The galaxy is moderately luminous, and there might be some signs of mild ongoing star formation activity. Overall, the galaxy presents as a mature system, likely situated within the 'red sequence' of galaxies.
