The galaxy appears as a largely spheroidal object with a smooth light distribution, suggesting an elliptical morphology. There is a concentration of light towards the center, indicative of a bulge. The galaxy exhibits a redder hue, potentially implying an older stellar population and lower levels of current star formation. The absence of clearly defined spiral arms or dust lanes further supports its classification as an elliptical galaxy. There is no indication of any recent major merger activity or significant tidal disturbances in this image, but there seems to be a slight, very nearby minor disturbance. The galaxy has an estimated size of approximately 10 kiloparsecs.
