The galaxy presents as an elliptical or lenticular morphology with a smooth, relatively featureless appearance. The central region exhibits a concentrated luminosity, appearing brighter and more yellow in color, indicative of an older stellar population. The outer regions fade into a bluish hue, suggesting the presence of younger, bluer stars in the galactic disk, albeit with very little apparent structure. There is a slight indication of a flattened shape, but the galaxy appears largely spheroidal. No obvious spiral arms or bar structures are discernible. There is no strong evidence of an ongoing major merger event, although some minor asymmetries or disturbances in the outer regions cannot be entirely ruled out.
