The galaxy presents a generally smooth, round morphology, with an approximate effective radius of 4.2 kpc. It exhibits a dominant central bulge, which emits strongly in the g-band. Faint disk features are present, but the disk structure is not prominent. There appears to be minor disturbance in the galaxy's morphology, likely due to a smaller companion galaxy or previous interaction. The blue color suggests ongoing star formation in a portion of the galaxy. Based on the morphology, it could be an early-type spiral galaxy, or a lenticular galaxy undergoing some star formation.
