The galaxy presents a predominantly smooth morphology, suggesting a relatively evolved system. It exhibits a roughly elliptical shape, appearing more elongated than circular, but without extreme elongation. There is no prominent spiral structure visible. The galaxy has a bright central region that gradually fades into the outer parts. While the overall appearance is smooth, there is a subtle hint of possible disturbances or faint features. There is no evidence of major ongoing merger activity, although the possibility of past minor interactions cannot be ruled out based on the image alone. The colors appear relatively uniform, without any obvious distinct color variations across the galaxy, suggesting a consistent stellar population.
