The galaxy appears as a relatively smooth, round object with a centrally concentrated light profile. There is a bright, diffuse core that fades into the outer regions of the galaxy. The color is generally bluish, indicating a younger stellar population, though some redder hues may be present towards the outskirts. There is no discernible spiral structure or prominent dust lanes visible in the image. The galaxy appears to be relatively undisturbed, showing no signs of ongoing major mergers, tidal tails, or strong morphological distortions. The galaxy is relatively compact in size. Based on the limited data from the single image, the galaxy may be classified as an elliptical or S0 galaxy. However, deeper imaging and spectroscopic data would be needed to fully classify the morphology and composition of this galaxy.
