The galaxy presents a primarily smooth and rounded morphology. There is a distinct central bulge, brighter and more concentrated than the surrounding area, which suggests a significant stellar population. The color of the bulge is slightly redder, potentially indicating an older stellar population with lower ongoing star formation compared to the outer regions. The galaxy is surrounded by a fainter, more diffuse halo or disk-like structure. The overall colour of the surrounding halo is bluer in appearance, suggesting the presence of younger stars and active star formation. The galaxy exhibits no obvious spiral arm structure or significant morphological disturbances, indicating that it is relatively undisturbed. There does not seem to be a particularly active central nucleus. Overall, the galaxy appears as a single, relatively undisturbed entity.
