The galaxy presents as a face-on spiral with a notable central bulge that appears yellow-white, indicating an older stellar population in this region. Distinct, though somewhat diffuse, spiral arms extend outwards from the central bulge. These arms exhibit a bluer hue, suggesting active star formation. There appears to be a moderate bulge size, with less distinct spiral structure toward the periphery. The galaxy shows no obvious signs of major tidal disturbances or ongoing mergers, although the spiral arms show some asymmetries. Overall, the galaxy appears as a relatively undisturbed, star-forming spiral galaxy at a considerable distance.
