The galaxy presents as a spiral, although it appears to be viewed at a significant angle relative to our line of sight, meaning that it is likely a disk galaxy with a central bulge. The central bulge appears relatively bright. Faint spiral arms extend outwards from this brighter central region, appearing fragmented. Overall the galaxy exhibits a blue hue, suggesting an active environment for star formation.  There is no obvious sign of a significant tidal disturbance indicating interaction with another galaxy, although subtle disturbances cannot be ruled out. A weak bar feature is also present.
