The galaxy presents as a dual-core system, potentially indicative of an ongoing or recently completed merger. The two cores exhibit different apparent colors; one appears more yellow, suggesting an older stellar population, while the other has a redder hue, possibly indicating a significant dust component or a younger stellar population obscured by dust. The overall morphology is disturbed, lacking a clear spiral structure or elliptical form. Faint tidal features or extended halos can be seen around the two cores, though their exact nature is difficult to determine given image resolution. The luminosity profile seems to be relatively compact with concentrated cores. The galaxy's light suggests moderate star formation activity, with the redder core likely contributing to the bulk of the present day starbirth. The general smoothness of the galaxy implies a system where major disruptions have already started relaxing into a more stable configuration. The roundness of the galaxy does not seem to have an easily determinable shape, with most of the light concentrated in the cores.
