The galaxy presents as a system with a possible interacting component. One component appears as a diffuse, elongated structure exhibiting a hint of disk-like morphology. Some patchy, irregular structures with varying color intensities are noted, particularly within the disk. These features suggest regions of active star formation. Another component appears as a more compact, relatively smooth and concentrated core. There is evidence of disruption in the form of tidal tails or bridges extending from the disk, possibly indicating gravitational interaction with the second, compact component. The overall color suggests the presence of both younger, bluer stellar populations and older, redder stellar populations.
