The galaxy presents a generally smooth morphology, with a centrally concentrated light distribution. The overall shape appears largely round, with only a slight deviation towards an elongated form. The light profile suggests a relatively featureless structure, lacking prominent spiral arms or distinct substructures. The dominant color is a yellowish hue, potentially indicating an older stellar population and a lower rate of ongoing star formation. There's no obvious signs of active merging or major tidal disturbances. Overall, the galaxy appears to be a relatively massive system with a population of primarily older stars, exhibiting a relaxed and relatively undisturbed state.
