The galaxy appears to be an elliptical galaxy, with a smooth, centrally concentrated light distribution. The core region is the brightest and most luminous. The galaxy exhibits a slight elongation. The color profile suggests a mature stellar population, with a redder hue overall. There is minimal evidence of spiral arms or dust lanes within the galaxy. The outer regions fade gradually into the background sky, making it difficult to determine the exact extent of the halo. It is not perfectly circular; the overall shape appears to be only slightly elliptical. There is a small possibility that the galaxy contains a minor disturbance, but it is hard to tell from this resolution.
