The galaxy presents as a centrally concentrated, relatively smooth object. Its morphology appears elliptical, with a high degree of central bulge dominance. There is minimal discernible disk structure or spiral arm features. The light distribution is quite regular, suggesting a relaxed system. There is evidence of some minor disturbances, but there are no signs of recent major mergers or violent interactions, although merging cannot be ruled out. The galaxy exhibits a color gradient, with the core appearing redder than the outer regions. The moderate redshift suggests this is an older galaxy. Overall, the system appears to be a massive, evolved galaxy with moderate to high star formation. 
