The galaxy appears as an elliptical structure, exhibiting a smooth and centrally concentrated light distribution. The core region presents a yellowish hue, suggesting a population of older stars. Progressing outward from the center, a gradual transition to slightly greener tones is observed, potentially indicating the presence of younger stellar populations or some ongoing star formation. The galaxy displays a moderate ellipticity, appearing more elongated than perfectly circular. No prominent spiral arms or distinct features such as dust lanes are discernible within the limitations of the image resolution. There might be faint tidal features visible but they are likely due to the blurring of the image. The overall morphology suggests a relatively evolved system, with a dominant spheroid component.
