The galaxy presents a largely smooth and rounded morphology. A slight elongation can be observed, though the galaxy is not significantly elongated. The light distribution is concentrated towards the center, with a gradual decrease in intensity outward. The galaxy exhibits a yellowish central region, transitioning to redder hues in the outer areas. No distinct spiral arms or bar structures are visible. There appear to be some minor irregularities in the light distribution, suggesting possible faint features or interactions, but the galaxy is primarily undisturbed. It exhibits a color profile indicative of an older stellar population and a low star formation rate. 
