The galaxy presents an elliptical morphology, exhibiting a smooth, featureless structure. The light distribution is concentrated towards the center, forming a bright, well-defined nucleus, while the outer regions display a gradual decrease in luminosity. The color profile indicates a dominance of older stellar populations, with a yellowish hue suggesting a lack of significant ongoing star formation activity. There is no apparent evidence of spiral arms or a prominent disk structure. The galaxy appears relatively undisturbed, lacking signs of recent major mergers or tidal interactions, although minor disturbances cannot be ruled out based on this image alone. The overall appearance points towards a relatively evolved galaxy.
