This galaxy presents as a relatively smooth, centrally concentrated object. The overall morphology appears elliptical. The central region exhibits a bright, yellowish core, which suggests a significant concentration of older stellar populations. Fainter, bluish extensions are visible surrounding the core, which indicate the potential for a small amount of ongoing star formation. There appears to be a slight disk-like structure. No prominent spiral arms or distinct features are readily discernible. The overall light distribution is relatively even and undisturbed, with no clear evidence of major tidal interactions or ongoing mergers. The red shift indicates it is a distant galaxy.
