The galaxy presents as a relatively smooth, single-component system. It exhibits a predominantly elliptical morphology, appearing generally round. The light profile seems fairly regular, with no strong indication of spiral arm structures. The galaxy's core region appears bright and concentrated, yellow in color, suggesting a population of older stars or significant dust obscuration. The outer regions of the galaxy fade gradually, with a hint of green around the edges. Overall, the galaxy does not exhibit signs of major ongoing merger activity or significant morphological disturbances, though there may be very minor disturbances.
