The galaxy presents as a concentrated spheroid, exhibiting a smooth, elliptical morphology. The central bulge dominates the structure, displaying a significantly higher surface brightness compared to the outer regions. A faint, diffuse halo extends outwards from the central region, gradually fading into the background. Subtle color variations are visible, with a tendency towards redder hues in the core, possibly indicating an older stellar population, and slightly bluer tints in the outer regions, suggesting some ongoing, but limited, star formation. No prominent spiral arms or distinct features are discernible, indicating a relatively passive galaxy. There may be some minor gravitational disturbances present, though no major mergers are apparent. The overall appearance suggests a large galaxy with minimal recent interactions and a predominantly old stellar population.
