The galaxy appears as a somewhat rounded, centrally concentrated object. Its color profile is generally yellowish-orange, suggesting an older stellar population. There is a bright central bulge. The smoothness of the light distribution indicates that this galaxy is likely an elliptical galaxy with a population of older stars. There appears to be a second object above the center of the main galaxy that appears to be interacting or in close proximity to the galaxy. Based on the overall smoothness and rounded appearance of the main galaxy, it may have undergone a past merger event which could be affecting the smaller object.
