The galaxy presents a generally smooth appearance, with a noticeable absence of well-defined spiral arms or a prominent central bar. It exhibits an elliptical shape. The light distribution suggests a centrally concentrated profile, decreasing in intensity gradually towards the outer regions.  The galaxy appears to be experiencing some form of gravitational interaction or tidal disturbance, as there is an irregular light distribution. The color gradients across the galaxy are subtle. A population of young, massive stars may contribute to the bluer hues in certain regions of the galaxy. This galaxy is experiencing some level of star formation.