The galaxy appears as a relatively smooth, concentrated object with a bright central bulge. Its overall shape is elliptical, with a moderate degree of roundness rather than being highly elongated. There are no apparent signs of strong spiral arm structures or a prominent disk. The light distribution is centrally concentrated, fading gradually outward from the core. The galaxy exhibits a color gradient, appearing bluer toward its outer regions and redder in the central bulge, indicating a possible variation in stellar populations, with younger, bluer stars potentially residing further out from the center, and older, redder stars congregating toward the core.

There are no obvious signs of major ongoing mergers or significant tidal disturbances, although there may be a very slight asymmetry or minor distortion. The overall appearance suggests a relatively evolved system, possibly undergoing relatively low levels of star formation. The galaxy exhibits a significant mass, indicating a developed stellar population.
