The galaxy exhibits a generally smooth morphology. The light is centrally concentrated, displaying a bright, diffuse core. The overall shape is largely elliptical to lenticular, deviating slightly from a perfect circle. There are some hints of faint, subtle extensions or distortions beyond the core, indicating the possibility of minor tidal interactions or internal dynamical processes. The galaxy presents a color gradient, with the core exhibiting a yellow-orange hue, transitioning to a bluer color in the outer regions. These color variations may indicate differences in stellar populations or dust content across the galaxy.
