The galaxy presents as a relatively smooth, elliptical morphology. It displays a concentrated central bulge, with a gradual decrease in luminosity outward from the core. The overall shape is nearly circular, showing minimal elongation. There's little evidence of spiral arm structure or distinct features, such as dust lanes or star-forming regions. A slight color gradient is observed, with the central bulge appearing more yellow, potentially indicating an older stellar population, while the outer regions exhibit a faint bluish hue. The galaxy seems largely undisturbed, showing no signs of major mergers or tidal distortions. Overall, the galaxy appears to be a passively evolving system.
