This galaxy presents as an interacting system. The primary galaxy appears to be a relatively luminous spiral, exhibiting a disk structure and a suggestion of spiral arms, though these features are somewhat obscured, giving the galaxy a somewhat smooth appearance. Its light is shifted towards the blue end of the spectrum.

There is evidence of tidal disturbance, perhaps a minor merger. This is indicated by the diffuse and irregular features extending from the main body, indicative of gravitational interaction with another galaxy.

A second, smaller galaxy is within close proximity, possibly undergoing interaction with the main galaxy. It has a more yellow/red hue, indicative of an older stellar population or higher dust content. The system displays a low star formation rate.
