The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that is a yellowish-orange hue, suggesting an older stellar population with reduced ongoing star formation. The galaxy displays a slight elongation, appearing more "in-between" than perfectly round or cigar-shaped. There appears to be little indication of significant recent mergers or major disturbances in its structure. A faint disk may be present. The galaxy seems to be relatively isolated.
