The galaxy presents as a centrally concentrated object with a largely smooth morphology. The dominant color is a yellow-orange hue, suggesting an older stellar population and/or significant dust obscuration. There may be faint indications of a weak disk structure or other features, but the overall appearance is predominantly smooth. The object appears largely undisturbed, showing no strong signs of on-going major merger activity, although some minor asymmetries or disturbances cannot be entirely ruled out. The shape of the galaxy appears closer to round than elongated.
