The galaxy presents a disturbed morphology, indicating a potential ongoing or recent merger event. There are clear signs of tidal disturbances, with elongated structures or tails extending from the main galactic body. The central region exhibits a bright, concentrated core, indicative of a significant stellar population. The overall color appears yellowish-white, suggesting a mix of stellar populations with a potentially dominant presence of older stars. Although difficult to discern in detail, the structure seems to lack a well-defined spiral arm structure, possibly due to the gravitational interactions disrupting any pre-existing spiral pattern. There is a subtle blueish tinge in some of the outer regions, suggesting a potential presence of younger, hotter stars perhaps forming in the tidal arms. The galaxy appears to have undergone, or is currently undergoing, a significant interaction that is shaping its morphology and influencing its stellar populations.
