The galaxy presents a mostly smooth and elliptical morphology, appearing moderately flattened. It exhibits a central bulge with a high degree of concentration that fades into an extended halo. Some faint, diffuse features are visible on one side of the galaxy, potentially indicative of minor disturbances or interactions. Color gradients across the galaxy suggest varying stellar populations, with the central region appearing bluer than the outer parts. The galaxy is primarily composed of an older, redder stellar population within its halo and has an overall intermediate luminosity.
