The galaxy appears to be a spiral type, though the spiral arms are not well-defined. The disk is not edge-on, but presented at an intermediate angle. The image indicates a low level of organized spiral structure.

The galaxy exhibits clumpy features, with several distinct regions of enhanced brightness scattered throughout the disk. These may be areas of active star formation. The central bulge is either small or non-existent. There is no strong central concentration of light in the nuclear region.

Based on the irregular and disturbed morphology, the galaxy may be undergoing a minor or major merger event. There are hints of tidal features or distortions in the outer regions, suggestive of gravitational interactions with another galaxy. Overall, this galaxy displays properties intermediate between a smooth elliptical and a well-defined spiral, showing signs of recent or ongoing interaction and star formation.
