The galaxy appears as a centrally concentrated, elliptical or spheroidal system with a smooth, diffuse light profile. Its color is predominantly yellow to orange, suggesting a population of older stars with lower rates of star formation. No distinct spiral arms or dust lanes are visible. The overall appearance suggests a galaxy with a high mass and a redshift of approximately 0.22. There are no visual signs of a major ongoing merger, though the possibility of minor disturbances or past merger events cannot be ruled out based solely on this image. The effective radius of the galaxy is relatively small.
