The galaxy appears to be a relatively smooth, moderately elliptical system. The light distribution suggests a centrally concentrated structure. There is a subtle elongation, but it is not highly flattened. There are some irregularities in its light distribution, potentially indicative of minor disturbances, though a merger event does not seem likely. The central region of the galaxy is distinctly brighter than the outer regions. The color of the galaxy indicates a population of older stars.
