The galaxy appears to be a relatively smooth, centrally concentrated object. Its overall shape is somewhat elliptical but close to round, exhibiting a moderate ellipticity. There are no obvious spiral arm structures or a prominent disk. There is a possible hint of asymmetry or minor disturbances in the outer regions. It displays a color gradient, with the central region appearing more yellowish, potentially indicating a population of older stars, while the outer regions show hints of bluer hues, possibly reflecting the presence of younger stellar populations.
