The galaxy presents a disk-like morphology, viewed at an oblique angle relative to our line of sight. There is evidence of a central bulge, which appears elongated along the major axis of the disk. The color gradient suggests active star formation. The disk appears somewhat disturbed, potentially indicative of minor gravitational interactions. The spiral structure is not well defined. There is a bright, somewhat smooth blue region, suggesting recent star formation, possibly triggered by the interaction. A reddish color is observed in the central regions of the disk. The galaxy displays a moderate degree of smoothness. No strong merging features are immediately apparent, but there is a slight asymmetry in the disk.
