The galaxy appears as a centrally concentrated, luminous object with an overall elliptical morphology. The core region exhibits a bright, yellowish-orange hue, suggesting an older stellar population. The galaxy's outer regions display a gradual decline in luminosity with hints of bluer color, which might indicate ongoing, but low, star formation in these areas, and possibly younger stars. There is a slight asymmetry in the outer halo. No prominent spiral arm structures or significant dust lanes are readily apparent in this image. The galaxy seems to be relatively undisturbed, showing no obvious signs of a major merger event, though there is a slight irregular halo suggesting possible minor interaction with another galaxy in the past.
