The galaxy presents a predominantly smooth morphology, suggesting an elliptical or lenticular type. A notable feature is its centrally concentrated light distribution, exhibiting a bright, yellowish core that gradually diminishes outwards. The overall shape appears roughly rounded, with a slight elongation. There is no obvious evidence of spiral arms or a prominent disk structure. Subtle color variations are observable, with the central region exhibiting warmer, yellower hues, potentially indicating an older stellar population, while the outer regions appear slightly bluer. The overall structure appears undisturbed, with no signs of major mergers or tidal disruptions.
