The galaxy presents a somewhat elliptical morphology, appearing as a disk galaxy observed at a considerable inclination. It exhibits a smooth, concentrated central bulge region that gradually transitions into a fainter, more diffuse disk. The overall color profile suggests a composite stellar population, with the bulge appearing more yellowish-orange, indicating older stellar populations, while the disk shows hints of bluer regions, possibly indicative of ongoing star formation. There are some disturbances or irregularities observable in the outer disk, but the central regions appear relatively undisturbed. It may be a more evolved spiral or a lenticular galaxy.
