The galaxy presents as a centrally concentrated spheroid with a diffuse, extended halo. The core region exhibits a yellowish hue, suggesting an older stellar population or significant dust obscuration. The outer regions of the galaxy display a bluer tint. Overall, the galaxy appears relatively smooth in structure, with no obvious spiral arms or strong irregularities. The morphology suggests the galaxy is likely an elliptical, potentially with a weak disk component. There are faint signs of disturbed morphology. Further, the elongation is moderate, indicating a flattened ellipsoidal shape with the semi-major axis oriented at an angle.
