The galaxy presents a disturbed morphology, exhibiting features suggestive of an ongoing or recent interaction. A pronounced central bulge is either absent, or very weak and possibly obscured. The dominant feature is a disk structure. Evident within the disk are structures that could be interpreted as spiral arms, though they appear somewhat disrupted. The galaxy shows irregular regions of enhanced blue emission, indicative of areas with elevated star formation. Some of the regions could be interpreted as HII regions. Faint tidal features and a slightly asymmetrical light distribution suggest possible gravitational influence from another galaxy. The color gradient indicates that the outskirts are generally bluer than the inner regions.
