The galaxy presents a largely smooth, elliptical morphology. It appears well-defined, with a centrally concentrated light profile exhibiting a gradual decline in luminosity towards the outer edges. The core region is bright, showing a yellow-orange hue that transitions to a reddish tint in the outer halo, suggesting an older stellar population and reduced levels of current star formation. There is little evidence of spiral arm structure or significant dust lanes. The object is mostly symmetrical, showing little to no major morphological disturbances or signs of ongoing merger activity. The galaxy exhibits a slightly elongated shape, with the major axis oriented roughly horizontally in the image.
