The galaxy presents a generally smooth, elliptical morphology with a bright, concentrated central bulge. The overall color profile suggests a population of older stars, evidenced by the yellowish-white hue in the core region. Surrounding the core, there's a diffuse, bluish halo, potentially indicating the presence of younger stars or ongoing star formation, though the activity appears relatively low. The galaxy exhibits a moderate degree of roundness, not appearing significantly elongated or distorted, suggesting it is likely a relaxed system without recent major merger events. There are some subtle irregularities in the outer regions, which could possibly suggest minor tidal interactions or internal disturbances. The galaxy's apparent size and brightness indicate that it is a moderately sized system.
