The galaxy presents a non-regular morphology, appearing as a complex system likely undergoing a significant interaction or merger. The central region exhibits a bright, concentrated core, possibly indicating a high density of stars or an active galactic nucleus. Evident is a tidal tail of stars that are yellow and seem to be spread out. There is a relatively small spiral arm visible. 

The overall color distribution suggests a mix of stellar populations, with the central regions displaying a redder hue, indicative of older stars. The apparent disruption of any spiral arm structure and the presence of a faint tidal feature support the hypothesis of an ongoing merger event.
