The galaxy presents as a relatively smooth, centrally concentrated object with a roughly elliptical morphology. The central region exhibits a bright, yellowish-white hue, suggesting an older stellar population dominating the light output. Fainter, bluish extensions are observed at the outermost edges, hinting at the presence of some younger stars or ongoing star formation, although at a comparatively low rate. There are no obvious spiral arm structures or prominent dust lanes visible. The overall appearance indicates a galaxy transitioning from an active star-forming phase to a more quiescent state. It shows a relatively high degree of symmetry and roundness, lacking any strong signs of recent or ongoing major merger events. Faint wisps or tidal features are weakly present, suggesting possible minor gravitational interactions or disturbances in the past.
