The galaxy presents a largely smooth, elliptical morphology. It appears approximately circular, with a diffuse outer halo. The central region exhibits a strong concentration of light, suggesting a prominent galactic nucleus. A slight color gradient is observable, transitioning from a bluer hue in the center to redder tones toward the outer edges. There is no obvious presence of spiral arms or a well-defined disk structure. No active merging or tidal disturbances are apparent, though there is a minor color disturbance on the outskirts, which may indicate minor ongoing interaction. This galaxy is relatively massive, with a moderate amount of star formation occurring within it.
