The galaxy presents as a largely featureless elliptical or lenticular structure. The core is bright and concentrated, exhibiting a yellowish hue suggesting an older stellar population. The outer regions fade gradually into the background, forming a relatively smooth halo. The galaxy appears to be mostly undisturbed, showing no signs of major mergers or tidal interactions. There is a slight elongation visible, suggesting the galaxy is not perfectly spherical. Overall, the morphology suggests a well-evolved galaxy with a low star-formation rate and a significant stellar mass.
