The galaxy exhibits a primarily smooth morphology. It appears approximately circular in shape, with a concentrated central bulge. The light distribution suggests a relatively uniform structure, though there are some subtle irregularities in the outer regions, potentially indicating minor disturbances. There are slight color variations, with a central region that appears somewhat yellower and a surrounding halo that tends toward blue. These colors indicate areas of active star formation and varying star ages. The galaxy does not show clear spiral arm structures or a distinct disk when observing its features. The data appears to be indicative of a merging event. 
