The galaxy presents as a relatively smooth, elliptical-like structure. It displays a concentrated central bulge, characterized by a yellowish hue, suggesting an older stellar population. The outer regions exhibit a more diffuse, fainter glow with hints of a greenish tint, possibly indicating some ongoing, albeit low-level, star formation. No prominent spiral arms or distinct features are readily apparent. The overall morphology suggests a galaxy that has largely completed its major evolutionary processes, with minimal signs of recent mergers or significant disturbances. It appears well-defined and isolated. The color gradient from the center outwards implies a radial variation in stellar age or composition. The round shape indicates that it is not a spiral galaxy. The light emanating from the galaxy appears to be slightly redshifted.
