The object presents as a spiral galaxy, seen at a near face-on orientation. There is a prominent central bulge, with a relatively high surface brightness, that appears more yellow in color, indicating an older stellar population. The disk is visible and shows evidence of spiral arm structure. Two main spiral arms appear to emanate from the central region, tracing outwards in a relatively grand design. The arms show bluer colors compared to the bulge, suggesting the presence of ongoing star formation. Dust lanes are subtly visible within the spiral arms. The overall shape indicates a galaxy with a relatively high concentration of mass in its central region. The galaxy appears relatively isolated, with no immediately obvious signs of tidal disturbances or interactions. 
