The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. There is a noticeable color gradient, transitioning from a yellowish-orange core to a bluer, more diffuse halo or outer region. The overall shape is generally rounded, showing minimal signs of significant disturbance or tidal interactions. Any disk features are absent. The galaxy appears to be a fairly isolated system, with no obvious indications of ongoing merger activity or major distortions in its morphology. The color distribution suggests a relatively old stellar population dominating the central regions, with potentially younger, bluer stars present in the outer regions. The extended halo is faint but visible, indicating a diffuse distribution of stars extending beyond the main body of the galaxy.
