The galaxy presents as a centrally concentrated object with a relatively smooth overall appearance. It exhibits a slightly elliptical morphology, deviating marginally from a perfect circle. The core is characterized by a bright, yellowish-white hue, indicating a likely concentration of older stellar populations. This central region gradually fades into a bluer disk, hinting at ongoing, albeit subdued, star formation activity in the outer regions. There is no compelling evidence of strong spiral arm structures or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed, with no clear signs of major ongoing mergers. Close inspection reveals a faint, diffuse halo extending beyond the main body of the galaxy.
