The galaxy appears to be a relatively smooth, elliptical system. Its central region exhibits a concentrated luminosity, suggesting a substantial stellar population and potentially a supermassive black hole actively accreting material. The overall color profile tends toward redder hues, indicative of an older stellar population and a lower rate of on-going star formation within the galaxy. There is a small amount of bluer light on the fringes, implying some lower level of star formation. The morphology suggests that it is an isolated galaxy. No obvious signs of tidal interactions or recent merger events are visible. The galaxy presents a largely undisturbed structure, which could imply a period of relative quiescence in its recent evolutionary history.
