The galaxy presents as a primarily smooth, elliptical object. The color profile exhibits a central concentration of bluer wavelengths, possibly indicating a region of younger stellar populations or ongoing star formation. Moving outward, the light appears to become redder, which may indicate an older population of stars. The overall morphology appears to be neither perfectly spherical nor highly elongated, suggesting an intermediate ellipticity. There is no strong evidence of a disk or spiral structure. Some visual asymmetry could indicate a minor gravitational disturbance or recent interaction with another galaxy, though the object is mostly undisturbed.
