The galaxy presents as a lenticular or early-type spiral. It has a smooth, centrally concentrated bulge that dominates the overall light profile. The galaxy exhibits an elongated shape, with a noticeable disk component. The disk is not highly resolved but appears relatively uniform in color, with hints of bluer regions that may suggest ongoing star formation. No strong spiral arm structures or bars are visible. Overall, the morphology suggests a galaxy in a transitional phase between a spiral and an elliptical, characterized by a significant stellar mass and a modest rate of star formation. There are minor signs of tidal disturbance suggesting there may be some interaction with another galaxy.
