The galaxy presents as a centrally concentrated, roughly circular object. Its light profile appears smooth with a significant fraction of its light originating from the central region, which diffuses outward in a continuous gradient. The galaxy's structure lacks any obvious spiral arms or bar features. There's a subtle hint of a diffuse, extended halo surrounding the main body of the galaxy. No obvious signs of a recent major merger are apparent, although there may be some subtle disturbances. The galaxy's color indicates a population of older stars, implying a relatively low star formation rate.
