The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white glow, suggesting an older stellar population dominating the inner region. There is a subtle decrease in luminosity moving outward from the core, but no defined spiral arms or disk structure are apparent. The surrounding halo is relatively faint and blends gradually into the background sky, with no obvious signs of tidal disturbances or ongoing major mergers. The galaxy exhibits a round shape. There is a slight hint of redder hues in the outer regions. Overall, this galaxy presents a well-defined, evolved system with a likely quiescent star formation history.
