The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing quite round. There is a color gradient visible, transitioning from a yellower hue at the core to a slightly bluer tinge in the outer regions. No prominent spiral arm structures or significant dust lanes are discernible. There appears to be minimal disturbance in its overall structure. The general morphology is indicative of a galaxy where star formation is not currently a dominant process.
