The galaxy presents as a largely featureless elliptical or lenticular structure, exhibiting a centrally concentrated brightness profile. The core is bright and gradually fades into a more diffuse halo. Color gradients are subtle, with a slightly bluer periphery possibly indicating the presence of younger stellar populations in the outer regions. There is no distinct spiral arm structure or prominent dust lane visible. The shape is generally elliptical, with a minor axis approximately 85% the length of the major axis, indicating some degree of flattening. It lacks signs of major interaction or recent merger events, appearing relatively undisturbed morphologically.
