The galaxy presents as a moderately sized, somewhat elongated structure. It exhibits a diffuse, bluish central region, potentially indicating the presence of younger stellar populations and ongoing star formation. The overall shape seems to be transitioning between elliptical and disk-like, possibly an intermediate or peculiar morphology. There are hints of minor disturbances or irregularities in its outer regions, suggesting possible past interactions or mergers. The galaxy appears relatively smooth, but with subtle internal features. The color gradients suggest a more centrally concentrated star formation activity with potentially older stellar populations in the outer regions. Overall, the galaxy seems to be in a relatively late stage of its life cycle, but possibly still undergoing some level of star formation.
