The observed galaxy presents as a face-on or nearly face-on spiral galaxy. A bulge component is evident, appearing moderately sized with a yellow-orange hue indicating an older stellar population. The spiral arms are readily visible, though somewhat tightly wound. Indications of a bar structure seem likely, with a slight elongation or distortion of the central bulge region. The disk appears relatively undisturbed with a noticeable spiral structure. Star formation seems to be occurring within the spiral arms, indicated by the bluer color. Overall, no significant signs of a major merger event or strong tidal disturbances are apparent.
