The galaxy exhibits an elliptical morphology, appearing as a flattened spheroid. It displays a smooth light distribution, suggesting a relatively uniform stellar population and minimal dust obscuration. The core region shows a higher surface brightness, indicating a concentration of stars. There is a slight color gradient, trending towards redder hues in the outer regions and a green hue in the central region, potentially indicating a difference in stellar age or metallicity. The galaxy's orientation is nearly edge-on from our line of sight, giving it a lenticular appearance.
