This galaxy, observed at a redshift of approximately 0.2, presents a morphology that is generally smooth and elliptical in appearance. The galaxy exhibits a central bulge with a yellowish hue, suggesting a population of older, redder stars. There is a hint of a faint, bluer disk component extending outwards from the central bulge, although the overall light distribution is dominated by the bulge. No obvious spiral arm structures are observed, though there may be minor disturbances or faint tidal features that cannot be confidently discerned due to image resolution. The roundness index is approximately 0.7, indicating that it is mostly round. Any sign of a major merger, is relatively low, suggesting the galaxy is not undergoing major interaction with another galaxy. Overall, it is likely a massive galaxy with a relatively low star formation rate. 
