The galaxy presents as a largely elliptical, smooth structure. There is a central bright bulge that decreases in intensity moving outwards. This bulge appears slightly elongated, deviating from a perfectly circular profile. Subtle color gradients are observed, transitioning from a slightly redder hue near the center to a somewhat bluer tint in the outer regions. There are no apparent spiral arms or significant dust lanes. The morphology suggests a galaxy undergoing relatively quiescent star formation. Overall, the galaxy exhibits minimal signs of recent mergers or major disturbances, maintaining a largely undisturbed form.
