This galaxy presents a complex morphology. The central region is relatively compact and exhibits a reddish hue, possibly indicating a population of older stars or significant dust obscuration. Surrounding this core, there's a more diffuse, irregular structure with bluish and greenish tinges. The blue suggests areas of more recent star formation, while the green may represent ionized gas. A large, dark patch partially obscures the central region, potentially indicating a significant dust lane or complex of molecular clouds. Overall, the galaxy does not show a well-defined spiral or elliptical structure. The irregular shape and disturbed appearance may suggest a recent or ongoing interaction with another galaxy, as there is possibly minor disturbance occuring. It is possible, however, that the shape could also be due to image artifacts. More data and analysis are required to fully understand the nature and evolutionary state of this galaxy.
