The galaxy presents an elliptical morphology, elongated along an axis oriented approximately east-west. Its central region is diffuse, displaying a smooth light distribution without apparent substructure. A color gradient is observable, with a redder hue concentrated towards the core and a bluer tint extending outward, suggesting a possible gradient in stellar populations or dust distribution. The galaxy lacks any obvious spiral arms or a prominent central bulge; the light is rather evenly distributed, reinforcing its classification as an elliptical.
