The galaxy presents as a slightly elliptical, disk-dominated system viewed at a moderate inclination. The central bulge exhibits a yellow-white hue, suggesting an older stellar population. Surrounding the bulge, the disk shows a color gradient transitioning to a bluer color, indicating regions of more recent or ongoing star formation. While generally smooth in appearance, there is a subtle suggestion of spiral arm structure with only a minor disturbance. The galaxy does not appear to be undergoing a major merger.
