This galaxy appears to be a disk galaxy, observed at an oblique angle. There is a prominent bulge that dominates its central region. The bulge exhibits a smooth, relatively featureless structure, appearing to be made up of older stars. A flattened disk is observed extending away from the bulge. This disk has a reddish hue and is significantly fainter than the bulge, suggesting an older stellar population with lower levels of ongoing star formation. There is a slight asymmetry or possible disturbance in the morphology of the disk. Though largely appears to be of a late type morphology, with a dominant bulge.
