The galaxy presents a largely smooth, elliptical morphology. It appears quite concentrated, with a bright, yellowish core that gradually fades towards the edges. There is little evidence of spiral arm structure or dust lanes within the galaxy's body. The overall color suggests a relatively old stellar population, with a reduced rate of ongoing star formation. There might be a subtle deviation from a perfect circular shape, but no major disturbances are apparent in this single image. This galaxy likely contains a substantial mass and appears to have settled into a relatively stable configuration.
