The galaxy presents as a relatively smooth, elliptical or lenticular structure, appearing largely round in shape. There is a central bulge region with a higher concentration of light and a yellowish hue, suggesting an older stellar population. The surrounding area shows a bluer color gradient, indicative of ongoing or recent star formation, though the overall light distribution appears relatively uniform. The galaxy exhibits no strong signs of spiral arms or significant dust lanes, and appears relatively undisturbed, with only minor possibilities of interaction with neighboring objects.
