The galaxy presents as a relatively smooth, elliptical structure. It appears moderately luminous, exhibiting a concentration of light towards the center, which suggests a prominent galactic nucleus. The overall color profile indicates a dominant population of older stars, leaning towards redder wavelengths. There is a slight possibility of a faint disk component, but the image lacks sufficient detail to confirm its presence. The galaxy shows no obvious signs of recent major merger activity, though a minor interaction or internal disturbance cannot be ruled out. The object displays a roughly round morphology, with minimal deviation from a circular shape.
