The galaxy exhibits a disk-like morphology, though it is not perfectly face-on. There is a central bulge region that appears to be moderately bright and somewhat amorphous. The disk component is more prominent, displaying a flattened structure. There are possible spiral arm segments, though they are not well-defined. The disk shows variations in color and brightness, suggesting differences in stellar populations or dust content across the galaxy. Some regions appear bluer, indicating the presence of younger stars, while other regions seem redder, which could be due to older stars or dust obscuration.

The outer edges of the galaxy are diffuse, making it difficult to determine its precise boundaries. There may be some tidal features or minor disturbances present, indicating possible gravitational interactions with other galaxies or past merger events. The color variations observed throughout the galaxy hint at a complex star formation history.
