The galaxy appears as a centrally concentrated object with a smooth light distribution, potentially indicative of an elliptical morphology. The core exhibits a bright, slightly yellowish hue. The light distribution decreases relatively smoothly outward from the center, with only faint extensions. There is a slight elongation evident, suggesting it may not be perfectly spherical. No distinct spiral arm structures or prominent dust lanes are discernible in the image, consistent with a more evolved galaxy type. There is no visual evidence of a major ongoing merger.
