The galaxy presents as a generally smooth, elliptical morphology. The central bulge exhibits a concentrated luminosity, characterized by a yellowish hue, suggesting an older stellar population. There is a subtle radial gradient in color, with the outer regions appearing slightly redder, further supporting the presence of aging stars. No distinct spiral arms or dust lanes are discernible. The overall form indicates a high degree of radial symmetry and does not display any obvious signs of major disturbances or ongoing merger events. The outer regions appear diffuse, gradually fading into the background sky.
