The galaxy presents an elliptical morphology, with a smooth, concentrated central bulge exhibiting a yellow-white hue. The outer regions display a more diffuse, flattened structure, with subtle color variations suggesting areas of potential star formation, although no distinct spiral arms or prominent dust lanes are apparent. Overall, the galaxy appears relatively undisturbed, lacking any obvious signs of ongoing merger activity or significant tidal features. Its color profile indicates a population of evolved stars dominating the central region, while bluer tones in the periphery suggest the presence of younger stellar populations. The galaxy exhibits a degree of ellipticity.
