The object in the frame appears to be a spiral galaxy. It exhibits a prominent central bulge region that is bright and yellow-white in color. From this central bulge, spiral arms extend outward, showing significant definition and winding moderately tightly around the central region. 

A distinct bar-like structure is present, running through the galactic center. The spiral arms appear to originate near the ends of the bar. The arms appear fairly symmetrical. There are at least two observable spiral arms, and it is possible to observe more than two. 

There appears to be a small amount of distortion, as the symmetry of the spiral arms appears to be slightly off, suggesting a potential minor gravitational interaction with another nearby object or evidence of a past merger. There is a central bright region, but the bulge is quite small compared to the rest of the galaxy. There appears to be little to no dust, so light is able to pass through the galaxy without being obscured.
