This galaxy presents as a fairly smooth, elliptical-like structure. It has an elongated shape, suggesting it is not perfectly spherical, with its longest axis approximately twice the length of its shortest. A bright, concentrated central region is visible, which likely hosts a significant population of older stars. The color of the central region appears yellowish-white, indicative of an aging stellar population. The outer regions of the galaxy exhibit a bluer hue, possibly due to the presence of younger, hotter stars. However, the overall color gradient from center to edge is relatively subtle, suggesting a gradual transition in stellar populations rather than distinct, separate regions of star formation. There are no prominent spiral arms or dust lanes visible in this image. There is no obvious tidal distortion or interaction with other galaxies. The galaxy appears to be relatively isolated and undisturbed.
