The galaxy presents as a primarily smooth, elliptical morphology, with a high degree of central concentration as indicated by the bright central bulge. There is a relatively subtle color gradient, transitioning from a yellowish-white core to a slightly bluer outer halo. Though largely featureless, there is a very slight suggestion of a disk structure embedded within the light distribution of the galaxy. No distinct spiral arms or strong irregularities are readily apparent. There are no indications of a major merger event, though there could be very minor disturbances. Overall, the galaxy appears to be in a relatively relaxed state.
