The observed galaxy presents an overall smooth morphology, appearing nearly round in shape. There is no significant presence of a disk structure or prominent features such as spiral arms. The light distribution is relatively uniform across the galaxy's body, with a slight concentration towards the center. No signs of major disturbances or ongoing mergers with other galaxies are immediately apparent, though the presence of minor disturbances cannot be completely ruled out. The galaxy exhibits a moderately bright intensity, which is indicative of relatively strong light emission in the observed wavelengths. There appears to be a gradual falloff of light intensity from the central region outward, with no obvious sharp edges to the galactic boundary. The galaxy's light appears slightly red-shifted.
