The galaxy presents as a centrally concentrated object with a largely smooth overall appearance. There is a slight elongation to its shape, though it tends toward being round.  No distinct spiral arms or bar structures are discernible within the galaxy's structure. There is a slight color gradient, transitioning from bluer hues in the central regions to redder hues in the outer parts. This hints at potential differences in stellar populations across the galaxy, with possibly younger, hotter stars dominating the core, and older, cooler stars populating the periphery. There are some slight hints of disturbances nearby, but overall it appears to be stable and not heavily undergoing a merger.
