The galaxy presents a smooth, elliptical morphology with no apparent spiral arms or disk structure. The core is a bright, concentrated region with a yellowish-orange hue, suggesting an older stellar population. The galaxy's overall shape is moderately elongated. The outer regions exhibit a gradual decrease in luminosity and have a bluer color, potentially indicating the presence of a younger stellar population or some residual star formation. No significant tidal features or signs of recent mergers are discernible.
