The galaxy exhibits a generally smooth, elliptical morphology. It presents a concentrated central bulge that graduates outward. The central region displays a yellowish hue, likely indicating an older stellar population dominating this area. Moving away from the center, the color shifts towards bluer tones, suggesting the presence of younger, hotter stars in the outer regions, although these are less prominent. There's no apparent spiral arm structure or any significant dust lane features are observed. The overall shape suggests a relatively relaxed system without signs of recent major merger activity.
