The galaxy presents a largely smooth and rounded morphology. It appears to be an elliptical galaxy, or potentially a spiral galaxy seen face-on with poorly defined spiral arms. The light profile gradually decreases from the center, indicating a lack of a distinct galactic nucleus. The galaxy exhibits a blue-ish white hue in its central region, possibly indicating the presence of a population of relatively young, hot stars, or a region of low extinction allowing the underlying stellar population to shine through. The galaxy is fairly isolated with no signs of interacting with any companion galaxies. Overall, this galaxy appears to be a relatively undisturbed system.
