The galaxy presents as a somewhat elliptical structure, appearing elongated rather than perfectly spherical. The central bulge exhibits a high surface brightness, suggesting a dense concentration of stars. A disk component is suspected, but less prominent; it appears that this galaxy has a low rate of star formation. The galaxy is smooth in appearance, with no apparent spiral arms or intricate dust lane structures visible in the image. Color gradients are subtle, with the central region appearing more yellow/white and the outer regions exhibiting a slight blue tinge. There is no strong evidence of ongoing mergers or major disturbances, although a minor asymmetry cannot be ruled out. The overall light distribution suggests an evolved stellar population.
