The galaxy presents as a somewhat elliptical form, with a smooth and concentrated central bulge. The disk component, if present, is not clearly resolved in this image. Color gradients suggest a higher concentration of older stellar populations towards the galactic center, indicated by the yellowish-orange hue. A faint, diffuse halo surrounds the main body of the galaxy. A small, redder region is observed on the periphery of the galaxy. Overall, the structure is relatively undisturbed, showing no major signs of recent merger activity, though the slight irregularity on the edge could indicate minor disturbances.
