The galaxy presents as a relatively smooth, elliptical morphology. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population. The light gradually fades from the center outwards, where the outer regions of the galaxy exhibit a bluer tint. The overall shape approximates to being in between round and slightly elongated. There are no obvious signs of spiral arms, distinct dust lanes, or active star formation regions visible in this image. The galaxy appears relatively undisturbed, showing no major distortions or signs of a recent merger event. The image is consistent with a mature galaxy with a dominant spheroidal component.
