The galaxy presents a generally elliptical morphology, appearing relatively smooth and well-defined. It exhibits a bright central bulge, yellowish-white in color, suggesting a concentration of older stellar populations. The bulge gradually fades into a more diffuse halo. There's minimal indication of spiral arm structures or significant dust lanes. The overall color profile indicates the potential presence of ongoing, albeit subdued, star formation activity; it may be a more quiescent galaxy. There are no obvious signs of a major merger or significant tidal disturbances.
