The galaxy presents as a relatively smooth, elliptical-like structure with minimal discernible features. It exhibits a concentrated, bright central region that gradually diffuses outwards, transitioning from a yellowish hue to a faint, reddish halo. No distinct spiral arms or bar structures are apparent. There is a slight asymmetry in the color distribution, with the reddish halo appearing more prominent on one side. Overall the galaxy appears to be an old system with little current star formation, that does not appear to be undergoing a merger.
