The observed galaxy presents a flattened, disk-like morphology. A prominent, relatively smooth central bulge is not easily discernible, and the overall structure appears disturbed. The galaxy exhibits multiple faint features, including a slight tail that could possibly represent a tidal disturbance. The color is consistent with older stellar populations. The luminosity appears relatively low in the green band, which can indicate a low star formation rate or significant dust obscuration. Overall, the galaxy could be classified as a merging system or galaxy experiencing tidal disruption. Further spectroscopic data would be required to confirm the merger hypothesis and measure the galaxy's redshift to establish its distance.
