The galaxy appears to be a generally smooth and rounded object. It exhibits an elliptical shape with a bright, concentrated central region. The core is a yellowish-white hue, suggesting a population of older stars. A less luminous extension or plume of similar color extends from the central region. This plume is much less pronounced. The overall color suggests that the stellar population is dominated by older stars, indicating a relatively low rate of recent star formation. There is evidence of possible disruption in the surrounding halo. Although largely smooth, the overall morphology suggests a galaxy that may have undergone a minor merging event. 
