The galaxy presents an overall smooth and rounded morphology. Its core appears bright and concentrated, with a yellowish-white hue. The outer regions exhibit a gradual decline in surface brightness, appearing more diffuse. A subtle color gradient is observed, transitioning from the yellowish-white core to a slightly bluer tint in the outer regions. No distinct spiral arms or prominent features are discernible, suggesting a relatively undisturbed structure. There are no obvious signs of active star formation, and no major merger events. The galaxy appears to be a relatively isolated system.
