The galaxy presents as a relatively smooth, elliptical-like structure. There appears to be a concentration of light toward the center, suggesting a prominent galactic bulge. The light distribution decreases gradually from the core outward with the overall shape appearing mostly round. There is a hint of blueish color detected in the outermost regions which could be indicative of some star formation. There is no apparent spiral structure, and no prominent tidal features or distortions are visible that would indicate a major merger event. However, a slight asymmetry in the outer light distribution might suggest a minor interaction or disturbance. Overall, the galaxy appears to be relatively isolated and undisturbed.
