The galaxy presents as a relatively smooth, elliptical morphology with minimal discernible substructure. The light distribution appears largely concentrated towards the center, exhibiting a gradual decline in intensity with increasing radial distance. The color index suggests a population of older stars, implying relatively low current star formation activity. While the overall shape is predominantly round, there is a subtle deviation suggesting a slight elongation. There is no indication of major mergers or tidal disturbances, though minor disturbances are possible.
