The galaxy exhibits a flattened, disk-like morphology with a clearly defined central bulge. The bulge appears relatively smooth and bright, suggesting a high concentration of stars, possibly an older stellar population. The disk component shows some irregularities and clumpy features, hinting at ongoing or recent star formation. The outer regions of the disk appear fainter and more diffuse, with some evidence of spiral arm structure, though not sharply defined. There are areas of blue light in the disk, indicative of the presence of young, hot stars. There may be some minor tidal disturbance present, but it is not substantial.
