This galaxy exhibits a relatively smooth morphology, with a dominant central bulge. The overall shape is elliptical, appearing more elongated than perfectly spherical. The bulge displays a concentrated luminosity gradient, suggesting a high stellar density. The outer regions of the galaxy show a gradual decrease in surface brightness, with some subtle indications of a possible faint disk component. There is a hint of bluer light in the outer regions that may indicate ongoing, albeit low-level, star formation. No major disturbances or signs of ongoing mergers are readily apparent; however, there might be minor distortions present. The galaxy presents an overall evolved, quiescent appearance.
