The galaxy presents an overall irregular morphology, with possible signs of tidal disruption. A somewhat concentrated central bulge is visible, exhibiting a diffuse, light blue hue, indicative of moderate star formation. Extending from the central bulge, there is a faint, elongated structure. This appears to be a disk. There are subtle disturbances within the disk. There are several features that suggest this galaxy may be merging with another. Faint tails or plumes are seen on one side of the galaxy. These could be evidence of tidal stripping.
