The galaxy presents as a generally smooth, rounded structure with a concentrated central region exhibiting a yellowish-white hue. The outer regions transition to a slightly greenish tinge. No distinct spiral arms or prominent dust lanes are discernible, suggesting either a lack of significant star formation within a disk component or that the galaxy is primarily spheroidal in nature. There's no obvious indication of ongoing merger activity or significant tidal distortions in its morphology. The overall appearance suggests a relatively evolved system.
