The galaxy presents as a centrally concentrated object, with a smooth, elliptical morphology. The central bulge exhibits a yellowish-orange hue, indicative of an older stellar population. The galaxy appears elongated, deviating somewhat from a perfectly circular shape. There is little evidence of spiral arm structure or significant dust lanes. Overall, the galaxy presents with a relatively smooth and uniform structure, with possibly a weak bar. The outer regions appear less distinct. There is no evidence of strong interactions or major mergers.
