The galaxy appears to be a complex system, possibly undergoing a merger or strong tidal interaction. At least two distinct nuclei are visible, with one appearing more compact and potentially more massive based on its higher intensity. A diffuse, irregular structure connects these nuclei, hinting at tidal tails or bridges of stellar material ejected during the interaction. There are also several regions of star formation, which are bright and knotty, distributed throughout the galaxy.

The overall shape is elongated and asymmetric, lacking a clear spiral or elliptical morphology. It does not appear to be a well-defined disk or spheroidal system. The galaxy exhibits a broad range of colors, with redder hues concentrated in the more compact nucleus and bluer tints scattered in areas of star formation and tidal features.

The system’s disrupted morphology suggests a relatively recent interaction event that is inducing the ongoing star formation activity.
