This galaxy presents as a relatively smooth, centrally concentrated object, with a slight elongation. There is no obvious spiral structure or bar. The color gradient suggests an older stellar population, with a yellowish-white core possibly indicating a concentration of evolved stars. The galaxy exhibits a diffuse halo, which fades into the background, suggesting a lower density of stars at larger radii. There is minimal evidence of active star formation in this image, implying that it is a relatively quiescent galaxy. There is no strong indication of tidal features or distortions, suggesting a relatively undisturbed evolutionary history. The object appears largely isolated, with no obvious signs of ongoing or recent mergers.
