The galaxy presents as a relatively smooth, disk-like structure. Its shape is noticeably elongated, with a length roughly twice its width. There is a central, bright bulge exhibiting a yellowish-white color. This likely indicates a high concentration of older stars. The disk surrounding the bulge shows a subtle color gradient, transitioning from a yellowish hue near the center to a slightly bluer tinge further out. This might be due to the presence of younger, hotter stars in the outer regions of the disk, suggesting ongoing or recent star formation. No prominent spiral arm structures or major disturbances are immediately apparent; however, there is an overall hazy quality to the image, potentially obscuring finer details.
