The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. It exhibits a yellow-orange hue, suggesting a population of older stars and a relative lack of ongoing star formation. There is minimal evidence of spiral arm structure or dust lanes. The galaxy appears relatively undisturbed, showing no significant signs of tidal interactions or recent mergers, although minor disturbances cannot be ruled out based on the image alone. The shape is more rounded than cigar shaped.
