The galaxy presents as a largely smooth, elliptical structure. Its color profile is primarily yellow-orange at the center, suggesting a population of older stars. There is a slight color gradient moving outwards, with the outer regions appearing marginally bluer. The light is centrally concentrated with a gradual decline in brightness as you move to the galaxy's edge. There is no readily apparent spiral structure, or indications of recent major merger activity such as tidal tails. There is a very subtle indication of a disk. Overall, the galaxy exhibits a concentrated morphology, with a high degree of central symmetry.
