The galaxy exhibits a morphology that appears to be undergoing significant disturbance. Its overall structure lacks a well-defined spiral or elliptical shape, indicating an irregular classification. There are prominent irregular features and asymmetries present in the galaxy's distribution of light. Patches of bluer light emission are observed, suggestive of active star formation regions. The galaxy's appearance may be due to the presence of tidal features or interaction. Based on the irregular features, this galaxy shows indications of a potential merger event.
