The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, yellowish hue, suggesting a population of older stars. The overall shape appears slightly elongated, but not highly so. There is a subtle color gradient transitioning from the yellowish center to a bluer outer halo, indicative of a younger, star-forming population in the outskirts. No prominent dust lanes or spiral arm structures are discernible, suggesting that star formation activity is low. The image lacks evidence of any recent major mergers or tidal disturbances. Overall, it has a very regular appearance.
