The galaxy presents as a somewhat elongated structure, with an apparent disk-like morphology. There is a smooth, centrally concentrated bulge region. The disk component exhibits a mottled appearance, indicative of potential spiral arm structures or irregular star formation regions. The color gradient across the galaxy shows bluer hues in some regions suggesting younger stellar populations. Overall, the galaxy seems to be somewhere between a spiral galaxy and a lenticular galaxy in its characteristics, and the high fraction of smoother features indicates that it is a fairly evolved galaxy. There is a hint of a possible minor disturbance to the structure, possibly due to a past or ongoing minor merger event.
