The galaxy appears as a centrally concentrated object. It exhibits a predominantly smooth morphology with some notable features suggesting potential disturbances. The primary body of the galaxy displays a roughly circular shape, deviating slightly from perfect roundness towards an intermediate form. There is an indication of possible interaction or merging activity, as suggested by asymmetrical features within the galaxy's structure. The galaxy exhibits a color gradient, transitioning from a bluer hue in the central regions to redder tones towards the outskirts. This color variation could indicate differing stellar populations and ongoing star formation processes.
