The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology.  The color is generally redder, indicating an older stellar population. There is a subtle elongation, suggesting a departure from perfect circularity, though it is primarily rounded. No distinct spiral arms or bar structures are apparent. Faint, diffuse extensions might be present in the surrounding halo, but the image resolution limits definitive confirmation. There is no evidence of any recent or ongoing major merger events, tidal tails, or other significant disturbances in the morphology.
