The galaxy presents a predominantly smooth and featureless morphology, suggesting an elliptical classification. Its overall shape appears moderately elliptical, with a high degree of central concentration of light. The core exhibits a yellowish-orange hue, indicating an older stellar population. Moving outward from the core, the galaxy displays a gradual decrease in surface brightness. There is little evidence of spiral arms or a distinct disk structure. The galaxy does not show any obvious signs of major ongoing mergers or significant tidal disturbances, though a minor irregularity may be present. The overall color suggests a relatively low star formation rate, consistent with a more evolved system.
