The galaxy appears to be a relatively smooth, elliptical-like structure. Its morphology is characterized by a diffuse, centrally concentrated light distribution with no obvious spiral arms or distinct features. The galaxy exhibits a moderate ellipticity, appearing somewhat elongated rather than perfectly circular. The color gradient across the galaxy is subtle, with a slightly bluer hue in the outer regions compared to the yellowish core, which may imply ongoing, albeit subdued, star formation activity. Overall, the galaxy displays an unperturbed morphology, suggesting it has not undergone any recent major mergers or significant interactions.
