The galaxy presents as a spiral type, observed at a near edge-on inclination relative to our line of sight. The disk exhibits a complex structure with notable features, including spiral arm segments. There appear to be patchy regions of enhanced star formation activity within these arms, indicated by their bluer color. The central bulge is relatively small. There are also several dust lanes obscuring some regions of the galactic disc, especially near the bulge. There may be a weak bar structure present. There are no signs of any major mergers occurring, though there is some indication of a minor interaction or disturbances within the galaxy's morphology.
