The galaxy presents a largely smooth and rounded morphology. There is a concentration of light towards the central region, appearing as a bright, somewhat diffuse core. This core seems to transition gradually into the surrounding galactic structure, with no sharply defined boundaries. The overall color profile appears subtly redder, particularly in the central region, indicative of an older stellar population. There may be a very faint, almost imperceptible disk component that is only hinted at, but it remains difficult to ascertain without more detailed imaging. No strong tidal features or major disturbances are visible, suggesting a relatively undisturbed evolutionary history.
