The galaxy presents as a roughly elliptical structure with a concentrated central bulge, although the shape appears more lenticular than perfectly spherical. The light profile is relatively smooth, suggesting a lack of significant spiral arms. The colouration of the central region is yellow to white, becoming slightly bluer towards the outer edges. There appears to be some substructure within the galaxy, potentially indicating minor disturbances or ongoing interactions. The overall appearance suggests a mature galaxy with an estimated stellar mass around 10^10 to 10^11 solar masses and moderate ongoing star formation.
