The galaxy appears as a relatively smooth, elliptical or lenticular structure. It displays a concentrated central bulge, with a gradual decrease in luminosity towards its outer edges. The morphology is largely undisturbed, suggesting it has not undergone any recent major mergers. However, a slight distortion is visible along one edge. This could potentially be the result of minor gravitational interactions with other objects in its environment.

The galaxy's color suggests a relatively old stellar population, with a higher concentration of redder, evolved stars. This indicates a lower rate of on-going star formation within the galaxy. The galaxy is relatively massive.
