The galaxy presents a flattened, disk-like morphology with a distinct central bulge. The color profile suggests a heterogeneous stellar population, with a bright, bluish-white core that likely indicates active star formation or an active galactic nucleus. This core is surrounded by a green disk of light, suggesting intermediate age stars or ionized gas. The outer regions of the galaxy exhibit fainter, less structured emission. There appears to be at least one disturbance in the morphology of the galaxy.
