The galaxy presents a largely elliptical morphology, appearing mostly smooth with a high degree of central concentration of light. There is little evidence of spiral arm structure or dust lanes. The overall shape tends towards being intermediate in roundness, and has a slight deviation from being perfectly circular, tending towards a more elongated shape. The color profile indicates a population of older stars, with a greater emission in the redder bands of light. There is no indication of a major ongoing merger event, although some minor disturbance in the outer regions is not ruled out. Estimated values indicate the presence of moderate to high mass levels. Star formation rates appear to be fairly low.
