The galaxy presents as a generally smooth, elliptical form, with a concentrated central bulge. There is a subtle elongation, deviating slightly from a perfectly circular shape. The core exhibits a yellowish-orange hue, indicative of an older stellar population. The outer regions fade into a less distinct halo, exhibiting a decrease in luminosity and potentially hinting at the presence of evolved stars and a reduced rate of star formation. There are no obvious signs of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, with no major mergers or tidal features readily apparent. Overall, the morphology suggests a galaxy nearing a more quiescent stage in its evolutionary lifecycle.
