The galaxy presents as a yellowish-orange, moderately luminous object. Its overall morphology appears relatively smooth and elliptical, with no immediately obvious spiral arm structure. The shape is slightly elongated, neither perfectly round nor highly flattened. There is a subtle gradient in color intensity, suggesting the central region is somewhat brighter. While there is no clear evidence of a major merger, a subtle asymmetry or distortion of the galactic disk hints at the possibility of a minor gravitational interaction or disturbance. There is no dust lane visible in the image.
