The galaxy presents a generally smooth and elliptical morphology. Its color profile indicates a dominant population of older stars, resulting in a yellowish-orange hue that intensifies towards the galactic center. The galaxy exhibits a moderately elongated shape, appearing more oblate than perfectly spherical. There is no readily apparent dust lane or spiral arm structure. Faint blue colors on the edge of the halo suggest the presence of a low level of star formation. The lack of obvious tidal features or distortions suggest the galaxy is not currently undergoing a major merging event. The galaxy is likely a massive system, given its apparent size and brightness. The overall structure and color index are consistent with an early-type galaxy.
