The galaxy presents as a flattened, disk-like structure, viewed at a moderate inclination. The central region exhibits a bright, concentrated bulge with a yellowish hue, suggesting an older stellar population. Moving outward from the center, the disk displays a smoother, less defined structure, with a subtle color gradient indicating the presence of some ongoing star formation activity. The overall form is relatively undisturbed, lacking any prominent tidal features or signs of a major merger event. The morphology appears generally smooth, with a large fraction of light coming from the central bulge. There is a slight elongation to the galaxy's shape.
