The galaxy presents as a fairly smooth, centrally concentrated object. Its morphology is predominantly elliptical or spheroidal, displaying a high degree of radial symmetry. The light profile appears diffuse, lacking prominent spiral arms or a distinct disk structure. The object exhibits an almost perfectly round appearance. There is no indication of any major mergers or significant tidal disturbances. The galaxy's color indices suggest a moderate amount of ongoing star formation, or at least a population of relatively young stars, but the colors are overall somewhat uniform across the galaxy's extent. No distinct features such as dust lanes or bright knots are discernible.
