The galaxy presents as a luminous, elliptical morphology. Its core region displays a high concentration of light, appearing as a bright, slightly elongated central bulge. The light distribution gradually decreases outward from the core, forming a diffuse halo with a smooth, featureless appearance. The overall color is shifted toward the redder end of the spectrum, which implies an older stellar population. The galaxy exhibits no apparent spiral arms, bars, or significant dust lanes. The shape of the galaxy is neither perfectly circular nor highly elongated, falling somewhere between a spherical and cigar shape. There are no signs of any major ongoing mergers or tidal disturbances, with a very faint suggestion of minor asymmetries in the outer regions.
