The galaxy presents as a centrally concentrated, smooth distribution of light, suggesting an elliptical morphology. It appears largely featureless, with no discernible spiral arms or bar structures. The color profile indicates a relatively older stellar population, with a yellow-red hue, consistent with a lack of recent star formation. The galaxy exhibits a high degree of circularity in its overall shape. There is no visual evidence of any ongoing major merger activity or significant tidal disturbances, but there may be a slight asymmetry suggesting minor interactions. The galaxy is fairly luminous, based on its apparent brightness.
