The galaxy presents as a generally smooth and elliptical object. The central region appears brighter and more concentrated, exhibiting a yellowish hue which could indicate an older stellar population with minimal ongoing star formation. The outer regions of the galaxy appear less luminous with a subtle fading towards the edges and a slightly greenish tint in the outskirts. There is no apparent structure such as spiral arms or a prominent disk. The overall shape is not perfectly spherical; there is a slight elongation, suggesting it might be classified as an elliptical galaxy that leans closer to a lenticular type. There are no obvious signs of tidal disturbances or ongoing mergers.
