The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a yellowish-white hue, suggesting a population of older stars. The outer regions display a more subtle blue tint, potentially indicating the presence of a younger stellar population, although its contribution seems minimal. There is no distinct spiral arm structure or pronounced dust lanes visible; the light distribution is diffuse and symmetric. The galaxy presents a generally regular and undisturbed appearance, showing little sign of ongoing or recent major mergers or tidal interactions.
