The galaxy presents a mostly smooth and rounded morphology, indicating a possible classification as an elliptical galaxy. The light distribution suggests a centrally concentrated spheroid with a gradual decrease in brightness towards the outer regions. There are some slight color variations in the galaxy. The central region appears more yellow, which may indicate an older stellar population. There is only slight evidence of any spiral arm structure or a pronounced disk component and the absence of significant dust lanes supports the hypothesis of it being an elliptical galaxy.
