The galaxy presents as a relatively smooth, elliptical-like structure. The core exhibits a high degree of central concentration, indicated by its bright, yellowish-white luminosity. Moving outwards from the core, the luminosity gradually decreases, fading into a more diffuse halo. There is little to no evidence of spiral arms or prominent dust lanes. The overall color suggests an older stellar population, consistent with a low star formation rate. The galaxy appears generally undisturbed, lacking any obvious signs of recent major merger activity. There are no indications of tidal tails or other morphological disturbances. The shape appears approximately round.
