The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits a generally elliptical morphology, with a round appearance. There is no readily apparent spiral structure or significant disk component visible in the image. The galaxy's core appears to be significantly brighter and more condensed than the surrounding halo, which diffuses outwards. There's a noticeable color gradient, with the core appearing bluer than the outer regions, hinting at possible differences in stellar populations. There are no signs of tidal disturbances or major mergers are observed. The overall structure suggests a relatively relaxed system.
