The galaxy appears as a moderately bright object with a roughly circular morphology. The light distribution suggests a relatively smooth profile, though with some subtle variations in brightness indicating possible faint features or irregularities in the disk. There is a slight central concentration of light, hinting at a possible bulge component, but it is not distinctly pronounced. The galaxy exhibits a blue hue, suggesting the presence of younger stellar populations and ongoing star formation. The overall structure suggests a disk galaxy, possibly of late-type, but without strong spiral arm definition. There is no obvious major merger activity, though subtle asymmetries could indicate minor disturbances or interactions with smaller companion galaxies.
