The galaxy presents as a generally smooth, elliptical structure. The central region displays a high concentration of light, suggesting a prominent bulge. Proceeding outwards from the core, the light intensity gradually diminishes into a diffuse halo. There is a subtle colour gradient visible, transitioning from a yellowish hue in the nucleus to bluer tones in the outer regions, which could possibly be caused by a slightly higher presence of more recent star formations in the outer halo. There is a slight hint of a disk component, but the overall form is dominated by the bulge-like appearance. The morphology appears undisturbed with no apparent ongoing major merger event.
