The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology leans towards elliptical, appearing mostly round with a slight deviation. The color profile indicates a presence of older stellar populations, trending towards redder hues, particularly within the core region. However, there is evidence of some recent star formation activity indicated by the presence of some bluer colors. There is no apparent spiral structure or prominent disk. The light is fairly symmetrical, showing no clear signs of ongoing major mergers or significant tidal disturbances.
