The galaxy presents as a centrally concentrated object with a relatively smooth light distribution, suggesting an elliptical morphology. The core region exhibits a bright, yellowish-white hue, possibly indicating an older stellar population. Moving outward from the core, there's a discernible transition towards a fainter, greenish-blue halo or disk component. This change in color could indicate the presence of younger, hotter stars within this outer region. The galaxy appears somewhat elongated, rather than perfectly spherical, suggesting a moderate degree of flattening. There's no obvious evidence of prominent spiral arms or significant tidal disturbances, indicating it may not be undergoing any major merger events. Overall, the galaxy appears relatively undisturbed.
