The galaxy presents as a slightly elongated spheroid, exhibiting a smooth, relatively featureless morphology. There is no immediately apparent spiral structure or strong evidence of active star formation regions through color variation; the light is dominated by a homogenous yellowish-white hue. The overall shape is neither perfectly spherical nor highly flattened, showing a moderate degree of ellipticity. There does not appear to be any indication of major mergers or significant tidal disturbances affecting the galaxy's structure. A minor asymmetry is observed in the light distribution but not enough to be indicative of ongoing mergers.
