The galaxy presents as a luminous, elliptical object. It exhibits a smooth, relatively featureless morphology with a high degree of central concentration. The light profile appears to gradually decline from a bright core outwards. There is no evidence of spiral arms or a prominent disk structure. The galaxy's shape is elongated. Minor distortions and disturbances appear to be absent in the image. The color gradient suggests a population of older stars, emitting light primarily in the redder wavelengths, though a central concentration of bluer light might be present.
