The galaxy presents as a somewhat diffuse, elliptical-like structure. Its core exhibits a higher surface brightness compared to its outer regions, indicating a concentration of stars toward the center. The galaxy appears mostly smooth in texture, with no prominent spiral arms or significant dust lanes visible. There is a slight elongation in its morphology, suggesting a deviation from a perfectly circular shape. Faint blue tinges are seen in the outer regions, indicating a potential presence of younger stellar populations, although this is not highly pronounced. There are no clear indications of any major ongoing merger events, but a subtle asymmetry hints at the possibility of minor gravitational interactions or past disturbances. Overall, the galaxy seems to be a relatively evolved system with a largely quiescent star formation rate.
