The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-orange, suggesting a population of older stars. The light distribution decreases gradually with increasing distance from the center. The galaxy shows a very slight elongation, appearing more "in-between" of round than a clear flattened disk. There is a hint of a minor disturbance in its overall structure. There is no clear spiral arm structure visible in the image.
