The galaxy presents as a smooth, elliptical-like structure. There is some irregularity in the morphology, indicating possible minor disturbances within the galaxy. The galaxy is dominated by redder hues, suggesting an older stellar population and relatively low ongoing star formation. The overall color profile indicates that the galaxy is not actively forming stars at a high rate and is likely in a more passive evolutionary state. There is the possibility of a very minor merger, or significant tidal distortions as suggested by some faint features.
