The galaxy presents a flattened, elliptical morphology, likely an oblate spheroid viewed at an angle. It exhibits a smooth, relatively featureless appearance, with a central concentration of light that diminishes gradually towards the edges. The core region displays a yellowish hue, potentially indicative of an older stellar population. The outer regions are less defined and exhibit bluer tones. There is no strong evidence of active spiral arms or significant dust lanes. The galaxy's overall structure suggests it could be an elliptical galaxy. There are no apparent signs of ongoing major mergers or significant tidal disturbances.