The observed galaxy presents a disturbed morphology, indicative of an ongoing or recent merger event. There are tidal tails emanating from the main galactic body, suggesting gravitational interactions. The color distribution shows regions of both older stellar populations, indicated by the redder hues, and younger, star-forming regions with bluer tones. The galaxy is not a pure disk or elliptical galaxy, but a more irregular shape. There is a secondary object that appears to be part of the merger, though it is not as defined as the primary component. This object is more compact and round, but still shows a disturbed morphology from the interaction with the primary galaxy.
