The galaxy appears to be an elliptical galaxy with a smooth morphology. The light distribution suggests a relatively even dispersion of stars, lacking any prominent spiral arms or a distinct central bulge. It exhibits a slightly elongated, cigar-like shape. The color profile indicates a population of older stars. Based on the observed color and lack of distinct features, star formation activity is estimated to be low. There is no obvious evidence of a recent or ongoing merger event, and the galaxy appears relatively undisturbed.
