The galaxy presents as a centrally concentrated, elliptical-like system. It exhibits a smooth, featureless morphology, with a high degree of central concentration. There is a slight elongation, appearing somewhat oval in shape, but not strongly so. The color profile indicates a relatively older stellar population, with a dominant yellowish-white hue in the core, which likely indicates the presence of older stars. Fainter blue is seen along the outskirts of the galaxy. No distinct spiral arms, bar structures, or dust lanes are evident. There is a suggestion of minor disturbance or possible recent interaction, given a slight asymmetry in the outer halo, however this needs further study. The overall appearance suggests a relatively evolved galaxy with quiescent star formation.
