The galaxy appears to be a relatively small, somewhat circular object. Its morphology is predominantly smooth, exhibiting a generally featureless structure with no apparent spiral arms or a distinct galactic disk. The color is a greenish hue, indicating the potential presence of ionized gases or active star formation. The galaxy's light distribution suggests a high degree of central concentration, with the brightness intensity gradually decreasing from the core outward. There is no obvious evidence of major mergers or significant tidal disturbances affecting its overall shape.
