The galaxy presents as a single, generally smooth object. Its morphology appears largely elliptical, with a high degree of circularity. No spiral arms or bar structures are discernible. The light distribution suggests a prominent central bulge that appears to have a yellow-orange hue. The outer regions exhibit a more diffuse, less luminous halo or envelope with a slightly greenish tint, suggesting the presence of a population of older stars. There's no visual indication of ongoing major merging events or strong tidal disturbances. The smooth nature and color profile indicates that the galaxy has a slow star formation rate.
