This galaxy presents a diffuse, irregular morphology, spanning an estimated angular size that would correspond to roughly 10 arcseconds on the sky. The light distribution is not dominated by a central bulge, and there is minimal evidence of a smooth, elliptical structure. Instead, the galaxy appears to be a composite of several distinct luminous regions.

These regions display varying colors, suggesting differences in stellar populations and/or dust content. Patches of blue light are apparent throughout the galaxy, which are indicative of star formation activity, and corresponding populations of young, hot stars. There are also areas with redder light which are indicative of older stellar populations.

The overall structure suggests either a disk galaxy with significant disturbances, or an ongoing galaxy merger. In particular, there are several areas which are not symmetrical.
