The observed galaxy presents as a spiral type, although there are signs of significant tidal disturbance. There are loosely wound spiral arms. The arms exhibit a clumpy morphology, which indicates active star formation. The galaxy possesses a prominent, moderately sized bulge. The bulge appears relatively smooth compared to the disk. A bar-like structure seems to be present, though its distinction is moderate. There is an indication of a possible merging event, or recent gravitational interaction with another galaxy, seen through the distorted morphology of the arms. The colours indicate a mix of stellar populations, with bluer regions associated with ongoing star formation. The redder regions appear to be more pronounced near the centre of the galaxy. The overall luminosity suggests this is a relatively large galaxy.
