The galaxy appears to be an elliptical type. It presents a smooth, relatively featureless morphology with a high degree of central concentration. The light profile appears uniformly distributed, indicating a well-mixed stellar population. The galaxy exhibits a pronounced spheroidal shape with a high degree of roundness, lacking any discernible disk or spiral arm structures. There are no obvious signs of recent major mergers or significant tidal disturbances. Color gradients suggest a dominant population of older stars, with a generally redder hue across the galaxy. The lack of blue regions indicates low levels of ongoing star formation activity. There is no apparent dust lane or patchiness. Overall, it seems to be an evolved galaxy, possibly nearing the red sequence.
