The galaxy presents a largely smooth morphology, suggesting an elliptical or lenticular type. Its structure is dominated by a central bulge exhibiting a high degree of circular symmetry. There is a subtle color gradient observable across the galaxy's surface, with a slightly bluer hue towards the outer regions, potentially indicating the presence of younger stellar populations at these locations. The relative absence of pronounced spiral arms or dust lanes suggests a system where star formation activity is not a dominant process currently. The overall light distribution is centrally concentrated, indicative of a mature galaxy where dynamical processes have had ample time to homogenize the stellar distribution. There is no clear indication of any significant ongoing or recent merger activity.
