The galaxy appears to be a relatively smooth and centrally concentrated system. It exhibits a generally elliptical morphology, with a high degree of roundness. There is no apparent spiral arm structure or prominent dust lanes visible. The galaxy’s light profile suggests a fairly smooth distribution of stars. Hints of a slight color gradient are present with a whiter center and slightly redder outskirts. There are no signs of active merging or major disturbances in the galaxy's structure, though minor disturbances cannot be fully ruled out.
