The galaxy presents as a relatively smooth elliptical or lenticular structure. The central bulge exhibits a yellow-orange hue, possibly indicating an older stellar population. The galaxy appears elongated, but is mostly round. There is a hint of a faint, extended disk or halo surrounding the brighter central region, with a subtle blue tint. This could indicate a small amount of ongoing star formation within that outer area. There is no obvious spiral structure, but there is a minor disturbance. The color suggests a general trend towards less star formation overall.
