The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a central bulge that appears yellowish-white, suggesting an older stellar population. The outer regions show a bluer hue, possibly indicative of younger stars or ongoing star formation, although this is not strongly pronounced. The galaxy's overall shape is elongated, with a hint of a disk-like feature, but the lack of well-defined spiral arms suggests a morphology somewhere between a pure elliptical and a spiral galaxy. There may be a hint of a minor disturbance in the outer edges of the disk, but overall the galaxy looks relatively undisturbed and non-merging.