The galaxy presents a generally smooth and rounded appearance. The central region displays a concentrated, yellowish-orange hue, suggesting a population of older stars. A subtle disk-like structure or feature is discernable, showing a bluish-green tint, potentially indicative of more recent star formation. There is no clear evidence of a major merger event, although some minor disturbances or interactions cannot be completely ruled out based on the image. The overall morphology suggests a transition between a truly elliptical galaxy and a spiral with a prominent bulge.
