The galaxy presents as a relatively compact object, exhibiting a smooth, centrally concentrated morphology. It appears largely spheroidal in shape, deviating only slightly from perfect circularity. The color profile suggests a dominant population of older stars, giving the galaxy a reddish-golden hue. There is no apparent structure indicative of spiral arms or a prominent disk. Faint hints of bluer regions may indicate areas of ongoing, but low-level star formation, particularly towards the outskirts. There are no signs of any major mergers. The surrounding halo appears relatively faint and diffuse, indicating a mature stellar population.
