The object presents as a relatively small, disk-shaped galaxy with a moderately bright core. There is a hint of spiral structure within the disk, though it appears quite disordered. The disk itself seems relatively thin and viewed at a high inclination. The light distribution suggests a relatively even mix of stellar populations across the disk. The galaxy appears somewhat disturbed, which could be due to an ongoing or recent minor merger event. Some tidal features may be present, but are unclear. The morphology is not strongly smooth, and has some signs of interaction.
