The galaxy appears to be a relatively smooth, centrally concentrated object. There is evidence of a disk. Color gradients indicate a possible radial variation in stellar populations, with the central region exhibiting a more yellow/red hue, suggestive of older stars, while the outer regions show a bluer tinge, indicating the presence of younger stars or ongoing star formation. The galaxy does not appear to be undergoing a major merger, but there are possible minor disturbances in its structure. 
