The galaxy appears to be a large, elliptical system, exhibiting a generally smooth and centralized light distribution. There is a dominant, bright central bulge. The galaxy's overall shape is moderately elongated, displaying an intermediate degree of ellipticity. There is no distinct disk structure, and the overall color index appears to be redder, suggesting an older stellar population and suppressed recent star formation. The morphology is indicative of a well-evolved galaxy without significant signs of recent mergers or major disturbances.
