The galaxy presents a primarily smooth morphology, with an overall elliptical shape. It exhibits a relatively high degree of central concentration, with a bright core that gradually fades into the outer regions. The color profile suggests a mature stellar population, with a dominant reddish hue, although a subtle blue tint can be observed within the central regions, potentially indicative of ongoing, albeit limited, star formation. There appears to be some disk-like structure. The galaxy does not appear to be significantly disturbed.
