The galaxy presents as a centrally concentrated object, appearing largely smooth in morphology. The core exhibits a bright, yellowish-white glow, suggestive of an older stellar population dominating the central region. Moving outwards from the center, a diffuse, blueish halo is observed, indicating the presence of some younger, hotter stars. There is a subtle suggestion of a disklike structure or feature. There is also no strong evidence of tidal tails or significant morphological disturbance, although some minor asymmetries are visible. The overall color profile suggests a mix of stellar populations, with a bias toward an evolved population in the central bulge.
