The galaxy presents as a relatively smooth, elliptical or lenticular morphology. The central bulge is bright and concentrated, exhibiting a yellowish hue suggestive of an older stellar population. A faint, diffuse disk surrounds the bulge, appearing somewhat elongated. There is some faint blue light in the galaxy, especially on the edges, which may indicate areas of recent star formation. The galaxy displays a slight asymmetry, which may suggest a minor gravitational interaction or internal disturbance. There are no obvious spiral arm structures or major merging features present.
