The galaxy presents as a disk galaxy, though the disk is not sharply defined, and the central bulge appears to be a significant component. The galaxy exhibits a moderate degree of internal structure. There is some evidence of spiral arms, but they are not tightly wound. They appear somewhat diffuse and ill-defined, giving the galaxy a slightly flocculent appearance. The galaxy appears mostly smooth, but there are minor disturbances. It shows some evidence of a slight asymmetry or warp. The galaxy has a notable red-shifted color, suggesting a significant distance. The axial ratio suggests it is not viewed perfectly face-on, and there is no strong evidence of an active galactic nucleus or a particularly high rate of star formation visible. There is no obvious sign of a major ongoing merger or tidal interaction, but there are some minor disturbances.
