This galaxy appears to be a relatively smooth, elliptical galaxy with a bright core. The galaxy exhibits a somewhat regular shape, showing a very minimal disk-like feature. The light profile suggests that it is primarily composed of older stellar populations, indicating a low rate of current star formation. There is a hint of minor disturbance in the galaxy's structure, but it does not suggest a major ongoing merger. The overall morphology suggests a galaxy that has largely completed its major evolutionary processes, settling into a relatively quiescent state.
