The galaxy presents as a roughly circular object with a high degree of central concentration. Its light profile appears smooth, lacking any obvious spiral arm structures or significant dust lanes. There is a slight elongation or distortion in the shape, but it is predominantly round. The galaxy's color index suggests a population of older stars, as indicated by its relatively redder appearance. There are no readily apparent signs of major mergers or significant tidal disturbances, though a minor asymmetry cannot be entirely ruled out.
