The galaxy presents an elliptical morphology, appearing mostly smooth with a high degree of central concentration. It exhibits a dominant bulge component, appearing more luminous and yellowish in color, suggesting an older stellar population. There is minimal evidence of spiral arms or a prominent disk structure. The overall color is somewhat muted, with a gradual transition from the brighter central region to a fainter, more diffuse halo. No significant dust lanes or signs of active star formation are readily apparent. The galaxy appears relatively undisturbed, with no obvious signs of a major merger event, though a small disturbance cannot be ruled out. It is moderately compact.
