The galaxy presents as a luminous, elliptical object. Its overall color is a pale yellow-white, suggesting an older stellar population. A subtle color gradient is observed, with the central region exhibiting a more pronounced yellow hue compared to the outer edges, which appear slightly bluer. This could indicate a more metal-rich population toward the galactic center. The galaxy lacks distinct spiral arm structures and appears relatively smooth. Its morphology suggests it is unlikely to be undergoing a major merger event. There are some areas that could be interpreted as minor disturbances, but this needs more study. The light distribution is centrally concentrated, with a gradual decline in surface brightness towards the outer regions, suggesting a de Vaucouleurs profile, typical for elliptical galaxies.
