The galaxy presents as a slightly elliptical, face-on or nearly face-on spiral system. The central bulge exhibits a bright, concentrated luminosity, suggesting a significant population of older stars. The disk component appears mottled and shows hints of spiral arm structure, though the arms are not sharply defined. The color gradient transitions from yellow-white in the core to a slightly bluer hue in the outer regions of the disk. A few faint, diffuse patches of blue light are observed within the disk, potentially indicative of areas of active star formation. The system displays no obvious signs of major mergers or strong tidal distortions. Overall, the galaxy appears to be a relatively undisturbed system with ongoing, but not exceptionally high, levels of star formation.
