The galaxy presents an irregular morphology. The core is characterized by a bright, concentrated region with a bluish hue, suggesting ongoing or recent star formation activity. Extending outward from the central bulge, the galaxy exhibits a less defined structure, indicating a non-smooth distribution of stellar populations. There are hints of asymmetry in the outer regions, possibly suggestive of minor tidal disturbances or interactions. A small, reddish extension is observed at the top, potentially indicative of a minor merger event or stellar debris. Overall, the galaxy appears to be experiencing some form of dynamical activity, resulting in its irregular shape and uneven distribution of color gradients.
