The galaxy presents a primarily disk-like morphology with a noticeable bulge. Spiral arm structures are clearly visible within the disk, appearing somewhat tightly wound. A bar is present running through the central region of the galaxy, and it appears to be of moderate intensity. The bulge appears to be moderate in size relative to the disk. There are hints of dust lanes or obscuration within the disk, and the galaxy is not undergoing any major merging events, although there may be some minor disturbances visible. Star formation seems to be relatively moderate. The galaxy exhibits a transition from bluer hues in the disk to yellower/redder colours within the bulge, which suggests an older stellar population in the center. The edge-on presentation is possible, but seems unlikely.
