The galaxy presents as a centrally concentrated object with a smooth, largely featureless morphology. The core exhibits a bright, concentrated luminosity. The overall shape is elliptical, with a slight elongation. The light distribution appears diffuse outwards from the core, indicative of a relatively old stellar population. There are no prominent spiral arms or dust lanes visible in the image. Color gradients suggest a redder central region compared to the outer regions. There is no indication of major ongoing star formation. The galaxy shows no obvious signs of a major merger.
