The galaxy presents as a moderately sized, irregular structure. Its light profile indicates a slightly elongated, disk-like morphology, although distinct spiral arms are not readily apparent. There is evidence of some internal structure, with a seemingly smoother central region gradually giving way to a more textured, diffuse outer region. The galaxy appears to be actively forming stars. A potential merging event could be distorting the shape of the galaxy. Overall, this galaxy exhibits a blend of smooth and irregular features, indicative of a possibly disturbed or dynamically evolving system.
