The galaxy presents an overall elliptical morphology, with a smooth, diffuse light distribution. The central region appears brighter and exhibits a yellowish-orange hue, suggesting an older stellar population. Moving outwards from the center, the color subtly shifts towards a slightly bluer tone, possibly indicating the presence of younger stars or ongoing star formation in the outer regions, but the difference is minor. The galaxy does not display any prominent spiral arms or distinct features, such as dust lanes. There is a very slight asymmetry in the halo region suggesting minor disturbances, but overall it appears to be a relatively undisturbed system. Based on the color, morphology and presence of star formation in the outer regions, it is likely to be in the process of transitioning into a more passive state.
