The galaxy presents a predominantly smooth morphology. Its light distribution is centrally concentrated, exhibiting a radial gradient that decreases outward from the core. There is a noticeable color gradient; the core appears more reddish, transitioning to a greenish hue in the surrounding regions. The galaxy appears largely undisturbed, lacking any obvious signs of recent major merger activity, although subtle disturbances may be present. Its overall shape is neither perfectly spherical nor highly elongated, suggesting an intermediate ellipticity. It appears to be a relatively massive galaxy with ongoing, albeit moderate, star formation.
