The galaxy appears to be a relatively face-on spiral or lenticular galaxy. It exhibits a prominent, bright central bulge with a yellowish hue, which likely indicates an older stellar population. The disk is visible extending from the central bulge, but is quite faint. The galaxy shows a high degree of smoothness in its overall structure, with only a few potential faint spiral arms. The galaxy is redshifted, indicating that it is fairly far from us and rapidly receding. There is some indication that it is not currently undergoing any major merging or tidal disturbance events. The bluer colors in the disk suggest ongoing though very low star formation. The galaxy is relatively massive.
