The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a higher concentration of light, appearing yellowish, suggesting an older stellar population. The outer regions are less defined, with a gradual decrease in luminosity. Faint blue hues are observed within the galaxy's halo, possibly indicative of ongoing, albeit low levels of, star formation. The galaxy shows a slight elongation, suggesting a shape somewhere between a sphere and a cigar. No obvious signs of tidal disturbances or major mergers are apparent. The overall appearance indicates a relatively relaxed, evolved system.
