The galaxy presents a generally smooth, elliptical morphology. Its color profile suggests a dominant population of older stars, exhibiting a yellowish-white core that fades into a bluer outer halo. There is a notable absence of defined spiral arms or dust lanes. The overall structure appears largely undisturbed, with no obvious signs of ongoing major mergers or tidal distortions. The central bulge is prominent and quite luminous. The galaxy appears to be relatively compact.
