The galaxy presents as a spiral galaxy with a distinct disk structure. A discernible central bulge is observed, appearing moderately sized. The galaxy is tilted relative to our line of sight, appearing somewhat edge-on. Faint spiral arms are apparent extending from the central bulge, though they are not tightly wound. The galaxy exhibits hints of possible disturbances to its overall morphology; perhaps a minor interaction is occurring. Overall, the galaxy appears to be a fairly massive galaxy with moderate ongoing star formation.
