The galaxy presents a largely smooth morphology, with a somewhat rounded appearance. There is evidence of a possible ongoing merger or interaction, with some structural distortion visible. The central region displays a bright, concentrated luminosity, potentially indicating a high density of stars or an active galactic nucleus. The galaxy exhibits a color gradient, with the central regions appearing bluer, suggesting a population of younger, hotter stars. Overall, the galaxy appears to be undergoing some form of dynamic interaction, influencing its structure and star formation activity.
