The galaxy presents a generally smooth, elliptical morphology. It displays a high degree of central concentration of light. The galaxy appears elongated, with a cigar-shaped structure. Its color profile transitions from a bluish-white core to a yellowish halo, suggesting a mix of stellar populations within its structure, with the core likely dominated by older stars. There are no obvious signs of spiral arms or active star formation regions. The galaxy does not appear to be strongly disturbed, and there are no indications of ongoing major mergers. Faint distortions are observed. 