The galaxy appears to be a luminous elliptical galaxy, displaying a generally smooth and rounded morphology. The dominant color is a yellow-orange hue, indicative of an older stellar population with fewer young, blue stars. There is no apparent spiral arm structure or distinct dust lanes. A slight asymmetry in the galaxy's outer isophotes may suggest a past minor merger event, or some gravitational interaction, though the central region remains largely undisturbed. Overall, the galaxy exhibits characteristics consistent with a well-evolved system with reduced current star formation activity.
