The galaxy presents a generally smooth, elliptical morphology, with a concentrated central bulge. The light profile appears diffuse, lacking strong spiral arm structures or prominent dust lanes. The galaxy exhibits a yellowish-white hue, indicating an older stellar population with a relatively low rate of recent star formation. There is a slight elongation visible, deviating from a perfectly circular shape. It appears to be relatively undisturbed, showing no obvious signs of major mergers or tidal interactions, though there may be slight distortions.
