The galaxy presents as a relatively smooth, elliptical-like structure. There is a prominent central bulge that appears bright, exhibiting a concentrated luminosity. The outer regions fade gradually, suggesting a diffuse halo. No distinct spiral arms or features of ongoing major mergers are visible in this image, suggesting a classification as an early-type galaxy. Faint blue hues exist in the outer region of the galaxy, potentially indicative of recent star formation, though the overall color profile tends towards redder wavelengths. The galaxy appears moderately round in shape. Based on the data, there may be the presence of minor disturbances, however these are not clearly discernible.
