This galaxy presents as a generally smooth, centrally concentrated structure. The color profile suggests a relatively evolved stellar population, with a dominant yellowish-red hue in the central region, indicative of older stars. There's a slight hint of bluer light in the outer regions, possibly suggesting ongoing star formation. The overall morphology is elliptical or possibly a tightly wound spiral seen nearly face-on, with a high degree of central concentration and a lack of easily discernible spiral arms or bar structure. There seems to be a very small disturbance to the shape of the galaxy, with no major asymmetries or tidal features visible. The galaxy appears relatively isolated.
