The galaxy appears as a centrally concentrated, relatively smooth object. Its light profile suggests an elliptical morphology, though it is not perfectly circular. The central region exhibits a bright, concentrated core, indicating a high density of stars. Surrounding the core, a diffuse halo extends outwards, fading gradually into the background. There is a slight blue tinge to the halo, potentially indicating the presence of younger stellar populations or ongoing star formation, but it is not particularly pronounced. There are no obvious spiral arm structures, bars, or tidal features suggestive of recent major mergers or disturbances. Based on its overall appearance, the galaxy could be classified as an early-type galaxy transitioning from a more active star-forming state.
