The galaxy appears as a centrally concentrated, elliptical object with a smooth, diffuse light distribution. It exhibits a yellowish hue towards the center, suggesting a population of older stars. Progressing outward, the galaxy shows a transition to a bluer color, hinting at the presence of younger stars in its outer regions. The galaxy's overall morphology indicates an evolved system, potentially lacking significant ongoing star formation in the nucleus. No distinct spiral arms or other features characteristic of disk galaxies are apparent. The shape is somewhat elongated, being less circular and more elliptical. There is no sign of any major ongoing merger events, nor any severe distortions. Minor disturbances in the morphology may be present.
