The galaxy presents as a primarily smooth and centrally concentrated object, exhibiting an elliptical morphology. Its overall shape is somewhere between a perfect circle and elongated like a cigar, appearing mostly in-between these shapes. A smooth light distribution suggests a relatively old stellar population. The galaxy exhibits a notable blue hue, concentrated in the central region which may suggest ongoing star formation in the galactic center. There is faint suggestion of minor asymmetry or a possible disturbance in the outer regions, although it is not a pronounced merger event.
