The object presents as a relatively compact galaxy, approximately estimated to be 9.7 units in radius. The galaxy exhibits an irregular morphology. A small percentage of the galaxy's light appears to be smooth, suggesting a possible central bulge or spheroidal component. However, a much smaller portion of the galaxy is showing signs of disk or features. Light analysis also indicates that a potential merging event or tidal interaction may be present, leading to its irregular form. A large portion of this galaxy has a chance of being an artifact.

In terms of color, there's a stronger presence in the blue and red channels, which suggest the presence of both young, hot stars and older stellar populations. It appears to be a somewhat actively evolving system with ongoing or recent disturbances affecting its overall structure.
