The galaxy presents a slightly elongated morphology. It exhibits a central bulge with a relatively smooth appearance. A disk is visible, displaying evidence of spiral arm structure, although details are somewhat indistinct. The overall color appears to be bluish, suggesting the presence of younger stellar populations and ongoing star formation. There are some irregular features that suggest possible gravitational interaction or disturbance. There is a hint of asymmetry in the outer regions, which may indicate a past or ongoing merger event.
