The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth and centrally concentrated morphology. The central bulge appears bright and yellowish-white, suggestive of an older stellar population. Moving outwards from the core, a slightly bluer and less concentrated halo extends. There is a noticeable absence of spiral arm structures or significant dust lanes, consistent with a galaxy dominated by older stars with little ongoing star formation. Some very minor disturbances might be present. The galaxy has a fairly round shape.
