The galaxy presents as a system undergoing a possible merger or strong tidal interaction. It appears to be composed of at least two distinct components. One component has a relatively smooth morphology, exhibiting a diffuse, round structure. The other component is more complex, displaying what appears to be irregular features and possible tidal tails or distortions.

The colors suggest varying stellar populations. The smoother component displays a slightly redder hue, potentially indicating an older stellar population. The complex component exhibits bluer regions, which may correspond to ongoing star formation. The overall color profile indicates a relatively young galaxy.

There may be a small concentration of yellower light near the center of the smoother component, suggesting either a central bulge or a region of concentrated older stars. The overall shape of the system is elongated, possibly due to tidal forces or gravitational interactions between the merging components. The system is not perfectly round, presenting as somewhat oblong. There appears to be some disturbance of the galaxy shape, which can potentially be attributed to a minor disturbance. A merging event may be occurring within the galaxy.