The galaxy appears to be a relatively smooth, elliptical type. The core exhibits a high degree of luminosity, appearing nearly spherical in shape with a concentrated central bulge. The light distribution suggests a lack of significant spiral arm structures. The color gradient across the galaxy shows a shift from a more reddish hue towards the center, transitioning to a yellow-greenish tint in the outer regions. There are no distinctly visible features indicating active galactic nuclei or substantial star formation regions, although the greenish hue may suggest some degree of recent star formation. There is a slight indication of a minor disturbance or asymmetry in its morphology. The overall appearance suggests a galaxy that is relatively evolved, with a dominant population of older stars concentrated towards the center.
