This galaxy exhibits a disturbed morphology, indicative of a potential merger event. A central, somewhat concentrated bulge region displays a yellowish hue. Extending from this core is a fainter, bluer disc-like structure, though its shape is irregular, showing asymmetries and possible tidal features. The outer regions of this galaxy appear disrupted, with extensions or plumes of material suggesting gravitational interactions. The galaxy is relatively bright, which is typical of galaxies with high star formation rates. Despite the signs of disruption, the presence of a bulge and a remnant disc suggests a classification of this galaxy as a disturbed spiral, possibly undergoing or having recently undergone a merging process.
