The galaxy presents as a spiral type, characterized by the presence of spiral arms. These arms appear somewhat diffuse and tightly wound, suggesting a classification toward the later end of the spiral sequence. The galaxy possesses a notable central bulge, visually moderate in size relative to the overall disk, and exhibits a bright, concentrated core. A bar-like structure seems to extend through the central region, indicating a barred spiral morphology. There is no noticeable inclination of the galaxy. The disk is well-defined, and the outer regions fade gradually into the background. No obvious signs of major mergers or significant tidal disturbances are apparent in the image. Color gradients suggest ongoing star formation within the spiral arms.
