The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated brightness, indicative of a dense stellar population, potentially an older population of stars given the yellowish-orange hue. The light appears to smoothly fade away from the center. The shape is moderately elliptical, tending toward round. There is no obvious spiral arm structure or prominent dust lanes visible. No significant morphological disturbances or merging features are detected. Overall, this galaxy appears as a quiescent, relatively undisturbed system, likely a mature elliptical galaxy.
