The galaxy presents a predominantly smooth, rounded morphology. Its overall structure appears largely undisturbed, lacking significant signs of ongoing or recent major mergers. The light distribution is concentrated, with a gradual decrease in intensity from the center towards the periphery. A subtle color gradient is observed, transitioning from a yellow/orange hue in the inner regions to a fainter greenish tint at the outer edges. The inner regions appear to lack active star formation, while the outer regions show faint signs of recent star formation activity.
