The galaxy presents a somewhat disturbed morphology. It appears elongated, with a noticeable asymmetry in its structure. The central region shows a concentration of light, possibly indicating a galactic nucleus or a bulge component. One side of the galaxy seems to exhibit a more diffuse and extended structure compared to the other, suggesting potential tidal interactions or ongoing mergers. There's a hint of bluer light in the galaxy, possibly due to the presence of younger stars and active star formation. However, the overall color appears relatively redder, indicating a population of older stars and a lower rate of star formation. Furthermore, based on its estimated size, it appears to be a relatively small galaxy, potentially a dwarf galaxy. The object seems to be undergoing some form of gravitational interaction, based on the morphology, but the nature of that interaction is not fully clear from the image alone. Further spectroscopic observations are needed to confirm its composition, star formation history, and merger status.
