The galaxy appears as a singular, centrally concentrated object. Its morphology is generally smooth and elliptical, with a high degree of central symmetry. There is a noticeable lack of significant features such as spiral arms or prominent dust lanes. The color profile suggests a moderate presence of older stellar populations, exhibiting a yellowish hue. There are no obvious signs of recent or ongoing major mergers, tidal tails, or strong gravitational disturbances, suggesting a relatively settled and unperturbed state. Overall, the galaxy presents a visual impression of a well-formed, early-type system with a dominant spheroid component.
