This galaxy presents as a spiral structure with a prominent central bulge. The spiral arms are clearly defined and extend outwards from the core region. A significant portion of the galaxy's luminosity is concentrated within the bulge, indicating a high stellar density in this region. The spiral arms exhibit moderate winding, suggesting an intermediate stage in the galaxy's evolutionary morphology. There may be two dominant arms. There are no significant signs of major disturbances or merging events, although subtle asymmetries in the outer disk could indicate minor interactions.
