The galaxy presents as a somewhat symmetrical, centrally concentrated system. The color profile is indicative of an elliptical morphology with a substantial population of older stars. The light is dominated by yellow and red wavelengths, and the galaxy exhibits a smooth appearance with a slightly elongated, though primarily round, shape. There is no discernible spiral structure or significant dust lanes within the system. Overall, the galaxy appears to be a passively evolving system with minimal ongoing star formation.
