The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears to be elliptical, with a high degree of roundness and no obvious disk structure visible in this image. There are no immediately apparent signs of tidal disturbances, major mergers, or strong asymmetries. The galaxy displays a redder hue, suggesting a population of older stars. Overall, the appearance indicates a spheroid-dominated galaxy with a fairly quiescent star formation history.
