The galaxy presents as a centrally concentrated object. It appears to have a smooth morphology, with a high degree of central light concentration and a spheroidal shape. The main body displays a fairly symmetrical light distribution. The galaxy's color index suggests a spectral energy distribution that may be composed of both old stellar populations and some degree of ongoing star formation. Overall, there are no obvious signs of major mergers or tidal disturbances in its morphology. Based on its apparent size and relatively smooth features, this appears to be a disk galaxy.
