The galaxy appears as a centrally concentrated, luminous object. It exhibits a relatively smooth morphology with a lack of discernible spiral arms or prominent features. The overall shape leans toward being somewhat round but could be classified somewhere between round and elliptical. There is a hint of radial color gradient, with a bluer tint at the center, suggesting the presence of a central population of younger stars. The galaxy does not display any obvious signs of major tidal disturbances or ongoing merger activity, although minor disturbances cannot be entirely ruled out based solely on this image.
