The galaxy presents as a roughly circular object, exhibiting a smooth, concentrated morphology. The light profile suggests a dominant central bulge. There's a slight suggestion of deviation from perfect circularity, but it appears largely featureless. The color suggests significant star formation. There appears to be a minor interaction with a secondary object, which is of significantly smaller size and shows up as a bluer shade. While difficult to discern, the host galaxy seems to have a significant concentration of star formation, which is concentrated in the central regions. The shape of the disk is mostly spheroid, with a slight cigar shape. It is not undergoing any significant merging events, though there is minor disturbance.
