The galaxy appears to be a relatively smooth, disk-dominated system, observed at an oblique angle. Its central bulge exhibits a yellowish-white hue, possibly indicating an older stellar population. Fainter disk extends from the central bulge outwards. There is a hint of blue in the outer regions of the disk, potentially suggesting ongoing star formation. The overall morphology suggests a relatively evolved system with some disk features. There is a very small amount of disturbance to the structure of the galaxy, as it is not perfectly symmetrical. 
