This galaxy appears to be a relatively smooth, elliptical system. The light is concentrated towards the center, forming a bright nucleus that fades gradually towards the outer edges of the galaxy. The color is primarily a yellow-orange hue, suggesting an older stellar population, with very little evidence of recent star formation activity and a corresponding lack of blue light. There appears to be no spiral arm structure and little indication of dust lanes or patchy regions of ionized gas within the galaxy. Overall, the morphology appears quite regular, with no significant signs of ongoing mergers or tidal disturbances.
