The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an overall elliptical morphology, presenting as mostly round in shape. There is a lack of any clear spiral arm structure or prominent dust lanes discernible in this image. The color distribution suggests an older stellar population is present, and is potentially undergoing a low level of star formation. The light profile appears smooth with no major disturbances that indicate on-going merger activity or strong tidal interactions.
