The galaxy presents a largely smooth, elliptical morphology with a concentrated central region. The light distribution indicates a high degree of spherical symmetry, with only subtle deviations suggesting minor structural features. It exhibits a color gradient, transitioning from a slightly bluer outer halo to a redder core, indicative of varying stellar populations across its radial extent. There is no evidence of spiral arms or a prominent disk structure. The overall appearance suggests a relatively evolved system with a substantial stellar mass and a low rate of ongoing star formation. Any potential interactions or disturbances appear to be minimal, as indicated by the lack of significant tidal tails or asymmetries.
